Mean magnitude and position on the discovery images:
2026 03 27.4426 2461126.9426 13.45 21:01:04.17 +40:06:36.4
82.59155 -4.07308 galactic Cyg Second-epoch detections are separated by 7.9" 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 J315.2558+40.1160 | 21:01:01.78 +40:07:11.5 (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 J315.2558+40.1160,2461126.9426,13.45,0.05,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
ATO J315.2558+40.1160 20260327.4426 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cyg-06-Q2b1x1_202117_TTUQ2b1x1_971_WWBcvjni/fd_Cyg-06-Q2b1x1_2026-03-27_05-36-48_20.00sec_-15.00C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cyg-06-Q2b1x1_202117_TTUQ2b1x1_971_WWBcvjni/fd_Cyg-06-Q2b1x1_2026-03-27_05-37-39_20.00sec_-15.00C_LIGHT_0494.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:04.17 +40:06:36.4 ;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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-27_05-37-39_20_00sec_-15_00C_LIGHT_0494_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_2026-03-27_05-36-48_20_00sec_-15_00C_LIGHT_0493_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_2026-03-27_05-37-39_20_00sec_-15_00C_LIGHT_0494_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_2026-03-27_05-36-48_20_00sec_-15_00C_LIGHT_0493_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4450 2461126.9450 12.01 18:25:03.84 +16:21:03.3
44.79946 13.08683 galactic Her Second-epoch detections are separated by 1.0" 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 | Gaia DR3 4522083349850465152 | 18:25:03.40 +16:21:05.1 (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 27.4450* 18 25 03.84 +16 21 03.3 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4522083349850465152,2461126.9450,12.01,0.05,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 4522083349850465152 20260327.4450 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20.00sec_-14.90C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20.00sec_-15.00C_LIGHT_0498.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:25:03.84 +16:21:03.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4450 2461126.9450 13.64 18:26:41.11 +17:11:24.1
45.74860 13.08595 galactic Her Second-epoch detections are separated by 4.4" 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 | ATO J276.6711+17.1880 | 18:26:41.11 +17:11:24.1 (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 27.4450* 18 26 41.11 +17 11 24.1 13.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J276.6711+17.1880,2461126.9450,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J276.6711+17.1880 20260327.4450 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20.00sec_-14.90C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20.00sec_-15.00C_LIGHT_0498.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:26:41.11 +17:11:24.1 ;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_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4450 2461126.9450 13.65 18:13:21.12 +13:45:34.9
41.15432 14.56336 galactic Oph Second-epoch detections are separated by 1.6" 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 | 18:13:21.12 +13:45:34.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=1.369+/- (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
target,2461126.9450,13.65,0.05,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 20260327.4450 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20.00sec_-14.90C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20.00sec_-15.00C_LIGHT_0498.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:13:21.12 +13:45:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4450 2461126.9450 13.78 18:52:09.03 +10:59:46.6
42.82229 4.83350 galactic Aql 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 J283.0387+10.9961 | 18:52:09.03 +10:59:46.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J283.0387+10.9961,2461126.9450,13.78,0.05,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
ATO J283.0387+10.9961 20260327.4450 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20.00sec_-14.90C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20.00sec_-15.00C_LIGHT_0498.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:52:09.03 +10:59:46.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4450 2461126.9450 13.62 18:33:09.11 +17:31:32.6
46.72465 11.82685 galactic Her Second-epoch detections are separated by 4.8" 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 4523946025628580608 | 18:33:09.83 +17:31:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 27.4450* 18 33 09.11 +17 31 32.6 13.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4523946025628580608,2461126.9450,13.62,0.05,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
Gaia DR3 4523946025628580608 20260327.4450 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20.00sec_-14.90C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20.00sec_-15.00C_LIGHT_0498.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:33:09.11 +17:31:32.6 ;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_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9450,13.45,0.05,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 20260327.4450 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20.00sec_-14.90C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20.00sec_-15.00C_LIGHT_0498.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:27:14.62 +11:00:13.3 ;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_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4450 2461126.9450 13.29 18:15:56.23 +15:42:03.2
43.24730 14.80810 galactic Her Second-epoch detections are separated by 3.7" and 0.4 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 J273.9847+15.7096 | 18:15:56.23 +15:42:03.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4450* 18 15 56.23 +15 42 03.2 13.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.9847+15.7096,2461126.9450,13.29,0.05,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
ATO J273.9847+15.7096 20260327.4450 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/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20.00sec_-14.90C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Her-10-Q2b1x1_203303_TTUQ2b1x1_3483_dnpQUlmp/fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20.00sec_-15.00C_LIGHT_0498.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:15:56.23 +15:42:03.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-41-02_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-10-Q2b1x1_2026-02-27_05-55-08_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-27_05-40-18_20_00sec_-14_90C_LIGHT_0497_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 11.77 19:49:10.30 +03:39:21.4
42.91817 -11.08744 galactic Aql Second-epoch detections are separated by 1.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.2865+03.6519 | 19:49:10.77 +03:39:23.7 (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 J297.2865+03.6519,2461126.9565,11.77,0.05,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
ATO J297.2865+03.6519 20260327.4565 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:10.30 +03:39:21.4 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 14.05 19:45:39.33 +03:56:49.7
42.75241 -10.17773 galactic Aql Second-epoch detections are separated by 1.0" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.4227+03.9511 | 19:45:39.33 +03:56:49.7 (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 J296.4227+03.9511,2461126.9565,14.05,0.05,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
ATO J296.4227+03.9511 20260327.4565 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:39.33 +03:56:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 13.16 19:22:41.06 +08:30:35.2
44.07473 -2.98970 galactic Aql Second-epoch detections are separated by 3.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J290.6644+08.5160 | 19:22:41.06 +08:30:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J290.6644+08.5160,2461126.9565,13.16,0.05,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
ATO J290.6644+08.5160 20260327.4565 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:22:41.06 +08:30:35.2 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 13.29 19:29:18.63 +03:00:11.5
39.96563 -7.02553 galactic Aql Second-epoch detections are separated by 0.2" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.3314+03.0019 | 19:29:18.63 +03:00:11.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.3314+03.0019,2461126.9565,13.29,0.05,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
ATO J292.3314+03.0019 20260327.4565 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:18.63 +03:00:11.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 12.80 19:38:11.60 +08:58:58.6
46.31954 -6.13663 galactic Aql Second-epoch detections are separated by 3.4" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.5408+08.9829 | 19:38:09.65 +08:58:26.2 (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 J294.5408+08.9829,2461126.9565,12.80,0.05,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 J294.5408+08.9829 20260327.4565 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:38:11.60 +08:58:58.6 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4565 2461126.9565 12.82 19:31:55.01 +04:56:57.9
42.00405 -6.68740 galactic Aql Second-epoch detections are separated by 1.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J193151.93+045705.9 | 19:31:51.92 +04:57:05.9 (Gaia DR3) | L (local) | (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 J193151.93+045705.9,2461126.9565,12.82,0.05,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
ASASSN-V J193151.93+045705.9 20260327.4565 12.82CV 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20.00sec_-15.00C_LIGHT_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aql-02-Q2b1x1_204211_TTUQ2b1x1_1200_jj8gY4i0/fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:55.01 +04:56:57.9 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-57-39_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-27_05-56-48_20_00sec_-15_00C_LIGHT_0517_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9634,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4634 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Sct-01-Q2b1x1_205815_TTUQ2b1x1_27340_f4N2PspP/fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20.00sec_-15.00C_LIGHT_0529.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Sct-01-Q2b1x1_205815_TTUQ2b1x1_27340_f4N2PspP/fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20.00sec_-14.90C_LIGHT_0530.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:31:54.10 -12:19:41.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20_00sec_-14_90C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20_00sec_-15_00C_LIGHT_0529_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20_00sec_-15_00C_LIGHT_0529_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4634 2461126.9634 13.02 18:51:09.28 -13:31:20.2
20.82011 -6.05887 galactic Sct Second-epoch detections are separated by 2.8" 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 4102195321130799360 | 18:51:10.77 -13:31:53.3 (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 4102195321130799360,2461126.9634,13.02,0.05,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 4102195321130799360 20260327.4634 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/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Sct-01-Q2b1x1_205815_TTUQ2b1x1_27340_f4N2PspP/fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20.00sec_-15.00C_LIGHT_0529.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Sct-01-Q2b1x1_205815_TTUQ2b1x1_27340_f4N2PspP/fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20.00sec_-14.90C_LIGHT_0530.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:51:09.28 -13:31:20.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20_00sec_-14_90C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20_00sec_-15_00C_LIGHT_0529_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20_00sec_-15_00C_LIGHT_0529_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9634,13.41,0.05,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
target 20260327.4634 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/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Sct-01-Q2b1x1_205815_TTUQ2b1x1_27340_f4N2PspP/fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20.00sec_-15.00C_LIGHT_0529.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Sct-01-Q2b1x1_205815_TTUQ2b1x1_27340_f4N2PspP/fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20.00sec_-14.90C_LIGHT_0530.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:41:35.15 -06:02:24.1 ;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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20_00sec_-14_90C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20_00sec_-15_00C_LIGHT_0529_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20_00sec_-15_00C_LIGHT_0529_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9634,14.23,0.05,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 20260327.4634 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/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Sct-01-Q2b1x1_205815_TTUQ2b1x1_27340_f4N2PspP/fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20.00sec_-15.00C_LIGHT_0529.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Sct-01-Q2b1x1_205815_TTUQ2b1x1_27340_f4N2PspP/fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20.00sec_-14.90C_LIGHT_0530.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:04:06.91 -08:53:50.1 ;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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20_00sec_-14_90C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20_00sec_-15_00C_LIGHT_0529_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-07-28_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-27_06-06-42_20_00sec_-15_00C_LIGHT_0529_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0922 2461128.5922 13.26 00:57:13.45 +59:16:05.5
123.67254 -3.59523 galactic Cas Second-epoch detections are separated by 2.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:57:13.45 +59:16:05.5 (user input) | T | P | (position from user input) J-Ks=0.706+/-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!
TCP 2026 03 29.0922* 00 57 13.45 +59 16 05.5 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.5922,13.26,0.05,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
target 20260329.0922 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cas-03-Q2b1x1_212336_TTUQ2b1x1_18266_6psn4CmG/fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20.00sec_-10.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cas-03-Q2b1x1_212336_TTUQ2b1x1_18266_6psn4CmG/fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20.00sec_-10.00C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:57:13.45 +59:16:05.5 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20_00sec_-10_00C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20_00sec_-10_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20_00sec_-10_00C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20_00sec_-10_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0922 2461128.5922 13.21 02:42:00.84 +63:11:08.6
135.02942 2.94109 galactic Cas Second-epoch detections are separated by 0.6" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:42:00.84 +63:11:08.6 (user input) | T | P | (position from user input) J-Ks=1.194+/-0.024 (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 29.0922* 02 42 00.84 +63 11 08.6 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,2461128.5922,13.21,0.05,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
target 20260329.0922 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cas-03-Q2b1x1_212336_TTUQ2b1x1_18266_6psn4CmG/fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20.00sec_-10.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cas-03-Q2b1x1_212336_TTUQ2b1x1_18266_6psn4CmG/fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20.00sec_-10.00C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:42:00.84 +63:11:08.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20_00sec_-10_00C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20_00sec_-10_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20_00sec_-10_00C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20_00sec_-10_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0922 2461128.5922 13.06 00:58:30.40 +57:44:44.4
123.87869 -5.11309 galactic Cas Second-epoch detections are separated by 3.4" 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 | ATO J014.6127+57.7420 | 00:58:30.32 +57:44:42.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.134+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.0922* 00 58 30.40 +57 44 44.4 13.1 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 J014.6127+57.7420,2461128.5922,13.06,0.05,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
ATO J014.6127+57.7420 20260329.0922 13.06CV 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cas-03-Q2b1x1_212336_TTUQ2b1x1_18266_6psn4CmG/fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20.00sec_-10.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cas-03-Q2b1x1_212336_TTUQ2b1x1_18266_6psn4CmG/fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20.00sec_-10.00C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:58:30.40 +57:44:44.4 ;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_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20_00sec_-10_00C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20_00sec_-10_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20_00sec_-10_00C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20_00sec_-10_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0922 2461128.5922 11.38 01:00:16.48 +58:34:54.8
124.08652 -4.27005 galactic Cas Second-epoch detections are separated by 1.2" 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 425720117623681280 | 01:00:16.55 +58:34:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.734+/-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!
TCP 2026 03 29.0922* 01 00 16.48 +58 34 54.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 425720117623681280,2461128.5922,11.38,0.05,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 425720117623681280 20260329.0922 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/Cas-03-Q2b1x1_2026-01-08_19-53-31_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-08_19-54-29_20.00sec_-14.90C_LIGHT_0017.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cas-03-Q2b1x1_212336_TTUQ2b1x1_18266_6psn4CmG/fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20.00sec_-10.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cas-03-Q2b1x1_212336_TTUQ2b1x1_18266_6psn4CmG/fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20.00sec_-10.00C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:00:16.48 +58:34:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20_00sec_-10_00C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20_00sec_-10_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-57_20_00sec_-10_00C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2026-01-08_19-53-31_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-28_21-12-09_20_00sec_-10_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_fd_Cep-03-Q2b1x1_2026-03-28_21-09-00_20.00sec_-10.00C_LIGHT_0005.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_fd_Cep-03-Q2b1x1_2026-03-28_21-09-00_20.00sec_-10.00C_LIGHT_0005.fits.cat
Mean magnitude and position on the discovery images:
2026 03 29.0894 2461128.5894 12.72 22:58:12.17 +67:33:33.4
112.42267 7.02786 galactic Cep Second-epoch detections are separated by 5.7" 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 2213076388545306880 | 22:58:11.62 +67:33:32.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2213076388545306880,2461128.5894,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2213076388545306880 20260329.0894 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-15_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q2b1x1_2025-12-26_20-10-55_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cep-03-Q2b1x1_212232_TTUQ2b1x1_14271_2ahfWQFe/fd_Cep-03-Q2b1x1_2026-03-28_21-08-13_20.00sec_-10.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cep-03-Q2b1x1_212232_TTUQ2b1x1_14271_2ahfWQFe/fd_Cep-03-Q2b1x1_2026-03-28_21-09-00_20.00sec_-10.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:58:12.17 +67:33:33.4 ;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_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-28_21-09-00_20_00sec_-10_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-28_21-08-13_20_00sec_-10_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-28_21-09-00_20_00sec_-10_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q2b1x1_2025-12-26_20-10-15_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png resample_wcs_fd_Cep-03-Q2b1x1_2026-03-28_21-08-13_20_00sec_-10_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 29.0965* 03 05 12.75 +46 48 26.0 14.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.5965,14.54,0.05,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 20260329.0965 14.54CV 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/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Per-02-Q2b1x1_212935_TTUQ2b1x1_5972_RPGfh1aK/fd_Per-02-Q2b1x1_2026-03-28_21-18-22_20.00sec_-10.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Per-02-Q2b1x1_212935_TTUQ2b1x1_5972_RPGfh1aK/fd_Per-02-Q2b1x1_2026-03-28_21-19-12_20.00sec_-10.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:05:12.75 +46:48:26.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png resample_wcs_fd_Per-02-Q2b1x1_2026-03-28_21-19-12_20_00sec_-10_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png resample_wcs_fd_Per-02-Q2b1x1_2026-03-28_21-18-22_20_00sec_-10_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_Per-02-Q2b1x1_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png resample_wcs_fd_Per-02-Q2b1x1_2026-03-28_21-19-12_20_00sec_-10_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png resample_wcs_fd_Per-02-Q2b1x1_2026-03-28_21-18-22_20_00sec_-10_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1070* 05 43 46.50 +08 11 52.9 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6070,13.71,0.05,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
target 20260329.1070 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/Ori-04-Q2b1x1_2026-02-21_20-50-02_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20.00sec_-10.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20.00sec_-10.00C_LIGHT_0035.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:43:46.50 +08:11:52.9 ;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_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_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_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_00C_LIGHT_0034_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1070 2461128.6070 12.78 05:42:46.06 +02:41:28.4
202.46994 -13.94531 galactic Ori Second-epoch detections are separated by 0.3" 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 | ATO J085.6969+02.6939 | 05:42:45.77 +02:41:33.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M3V 2015A&A...577A.128A HD 38014 B
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 29.1070* 05 42 46.06 +02 41 28.4 12.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.6969+02.6939,2461128.6070,12.78,0.05,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
ATO J085.6969+02.6939 20260329.1070 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q2b1x1_2026-02-21_20-50-02_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20.00sec_-10.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20.00sec_-10.00C_LIGHT_0035.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:46.06 +02:41:28.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_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_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_00C_LIGHT_0034_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1070 2461128.6070 13.19 06:20:43.67 +10:00:07.6
200.53260 -2.17178 galactic Ori Second-epoch detections are separated by 2.7" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3330486764252050560 | 06:20:43.98 +09:59:33.9 (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!
TCP 2026 03 29.1070* 06 20 43.67 +10 00 07.6 13.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3330486764252050560,2461128.6070,13.19,0.05,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
Gaia DR3 3330486764252050560 20260329.1070 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/Ori-04-Q2b1x1_2026-02-21_20-50-02_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20.00sec_-10.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20.00sec_-10.00C_LIGHT_0035.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:43.67 +10:00:07.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_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_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_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!
TCP 2026 03 29.1070* 05 36 23.87 +01 59 42.6 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6070,13.68,0.05,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
target 20260329.1070 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q2b1x1_2026-02-21_20-50-02_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20.00sec_-10.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20.00sec_-10.00C_LIGHT_0035.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:23.87 +01:59:42.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_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_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_00C_LIGHT_0034_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1070 2461128.6070 12.44 05:39:02.46 +05:12:56.0
199.73454 -13.52632 galactic Ori Second-epoch detections are separated by 0.3" 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 3332702280176925440 | 05:39:02.36 +05:12:54.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.115+/-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!
TCP 2026 03 29.1070* 05 39 02.46 +05 12 56.0 12.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3332702280176925440,2461128.6070,12.44,0.05,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 3332702280176925440 20260329.1070 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q2b1x1_2026-02-21_20-50-02_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q2b1x1_2026-02-21_20-50-52_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20.00sec_-10.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20.00sec_-10.00C_LIGHT_0035.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:02.46 +05:12:56.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_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_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_00C_LIGHT_0034_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1070 2461128.6070 13.05 05:39:47.58 +02:58:18.5
201.84617 -14.45984 galactic Ori Second-epoch detections are separated by 1.5" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:39:47.58 +02:58:18.5 (user input) | T | P | (position from user input) J-Ks=0.669+/-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!
TCP 2026 03 29.1070* 05 39 47.58 +02 58 18.5 13.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6070,13.05,0.05,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
target 20260329.1070 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q2b1x1_2026-02-21_20-50-02_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q2b1x1_2026-02-21_20-50-52_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20.00sec_-10.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_213534_TTUQ2b1x1_5398_F7swIVbl/fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20.00sec_-10.00C_LIGHT_0035.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:47.58 +02:58:18.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_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_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-15_20_00sec_-10_00C_LIGHT_0035_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-33-33_20_00sec_-10_00C_LIGHT_0034_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1028 2461128.6028 13.41 07:11:36.09 -13:10:18.4
226.93108 -1.59089 galactic CMa Second-epoch detections are separated by 7.2" 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 3044636968216121600 | 07:11:37.36 -13:10:14.9 (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 3044636968216121600,2461128.6028,13.41,0.05,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 3044636968216121600 20260329.1028 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/Mon-05-Q2b1x1_2026-03-19_21-12-03_20.00sec_-14.90C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Mon-05-Q2b1x1_213736_TTUQ2b1x1_10259_A5KEDm9j/fd_Mon-05-Q2b1x1_2026-03-28_21-27-25_20.00sec_-10.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Mon-05-Q2b1x1_213736_TTUQ2b1x1_10259_A5KEDm9j/fd_Mon-05-Q2b1x1_2026-03-28_21-28-12_20.00sec_-10.00C_LIGHT_0027.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:36.09 -13:10:18.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q2b1x1_2026-03-19_21-12-03_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Mon-05-Q2b1x1_2026-03-28_21-28-12_20_00sec_-10_00C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q2b1x1_2026-03-19_21-12-03_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Mon-05-Q2b1x1_2026-03-28_21-27-25_20_00sec_-10_00C_LIGHT_0026_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q2b1x1_2026-03-19_21-12-03_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Mon-05-Q2b1x1_2026-03-28_21-28-12_20_00sec_-10_00C_LIGHT_0027_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q2b1x1_2026-03-19_21-12-03_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Mon-05-Q2b1x1_2026-03-28_21-27-25_20_00sec_-10_00C_LIGHT_0026_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1028 2461128.6028 12.84 06:45:46.20 -07:06:41.7
218.63067 -4.49031 galactic Mon 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 | NSVS 12573351 | 06:45:45.39 -07:06:09.0 (Gaia DR3) | L: (local) | (local) | Gaia3var=VARIABLE SpType: M4 1993yCat.3170....0M IRAS 06433-0702
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12573351,2461128.6028,12.84,0.05,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
NSVS 12573351 20260329.1028 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-05-Q2b1x1_2026-03-19_21-12-03_20.00sec_-14.90C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Mon-05-Q2b1x1_213736_TTUQ2b1x1_10259_A5KEDm9j/fd_Mon-05-Q2b1x1_2026-03-28_21-27-25_20.00sec_-10.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Mon-05-Q2b1x1_213736_TTUQ2b1x1_10259_A5KEDm9j/fd_Mon-05-Q2b1x1_2026-03-28_21-28-12_20.00sec_-10.00C_LIGHT_0027.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:45:46.20 -07:06:41.7 ;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_Mon-05-Q2b1x1_2026-03-19_21-12-03_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Mon-05-Q2b1x1_2026-03-28_21-28-12_20_00sec_-10_00C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q2b1x1_2026-03-19_21-12-03_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Mon-05-Q2b1x1_2026-03-28_21-27-25_20_00sec_-10_00C_LIGHT_0026_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q2b1x1_2026-03-19_21-12-03_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Mon-05-Q2b1x1_2026-03-28_21-28-12_20_00sec_-10_00C_LIGHT_0027_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q2b1x1_2026-03-19_21-12-03_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Mon-05-Q2b1x1_2026-03-28_21-27-25_20_00sec_-10_00C_LIGHT_0026_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0909 2461128.5909 11.39 08:02:23.53 -29:46:34.7
247.16688 0.51036 galactic Pup Second-epoch detections are separated by 3.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5597057588952216448 | 08:02:24.81 -29:46:26.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B3/5 1975A&AS...21..193N [N75] 139
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5597057588952216448,2461128.5909,11.39,0.05,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 5597057588952216448 20260329.0909 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-02-26_22-17-06_20.00sec_-14.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20.00sec_-10.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20.00sec_-10.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:02:23.53 -29:46:34.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0909 2461128.5909 12.79 08:04:00.91 -29:59:58.1
247.54301 0.68952 galactic Pup Second-epoch detections are separated by 1.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5596660562178760192 | 08:04:00.02 -30:00:13.1 (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 5596660562178760192,2461128.5909,12.79,0.05,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 5596660562178760192 20260329.0909 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-02-26_22-17-06_20.00sec_-14.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20.00sec_-10.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20.00sec_-10.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:00.91 -29:59:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0909 2461128.5909 13.15 07:56:15.20 -30:10:06.9
246.80310 -0.82717 galactic Pup Second-epoch detections are separated by 1.6" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5597170838648087296 | 07:56:16.55 -30:09:56.7 (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 5597170838648087296,2461128.5909,13.15,0.05,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 5597170838648087296 20260329.0909 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/Pup-02-Q2b1x1_2026-02-26_22-17-06_20.00sec_-14.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20.00sec_-10.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20.00sec_-10.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:56:15.20 -30:10:06.9 ;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_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0909 2461128.5909 13.11 07:54:23.33 -26:15:00.9
243.23766 0.84928 galactic Pup Second-epoch detections are separated by 1.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5602078779368277888 | 07:54:25.30 -26:14:58.7 (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 5602078779368277888,2461128.5909,13.11,0.05,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 5602078779368277888 20260329.0909 13.11CV 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/Pup-02-Q2b1x1_2026-02-26_22-17-06_20.00sec_-14.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20.00sec_-10.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20.00sec_-10.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:54:23.33 -26:15:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0909 2461128.5909 13.31 07:34:16.13 -25:12:19.7
240.06916 -2.55471 galactic Pup Second-epoch detections are separated by 5.4" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J113.5658-25.2052 | 07:34:14.89 -25:12:45.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.338+/-0.063 (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 J113.5658-25.2052,2461128.5909,13.31,0.05,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
ATO J113.5658-25.2052 20260329.0909 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/Pup-02-Q2b1x1_2026-02-26_22-17-06_20.00sec_-14.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20.00sec_-10.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20.00sec_-10.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:34:16.13 -25:12:19.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0909 2461128.5909 13.70 07:17:17.56 -25:26:19.1
238.46579 -6.04963 galactic CMa Second-epoch detections are separated by 5.4" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J109.3263-25.4406 | 07:17:17.56 -25:26:19.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.3263-25.4406,2461128.5909,13.70,0.05,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 J109.3263-25.4406 20260329.0909 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/Pup-02-Q2b1x1_2026-02-26_22-17-06_20.00sec_-14.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20.00sec_-10.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20.00sec_-10.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:17:17.56 -25:26:19.1 ;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_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.5909,13.52,0.05,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 20260329.0909 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/Pup-02-Q2b1x1_2026-02-26_22-17-06_20.00sec_-14.90C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20.00sec_-10.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-02-Q2b1x1_214136_TTUQ2b1x1_25524_Dt6dQC52/fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20.00sec_-10.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:08:09.42 -29:56:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-11-10_20_00sec_-10_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-02-26_22-17-06_20_00sec_-14_90C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-28_21-10-17_20_00sec_-10_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0937 2461128.5937 13.20 08:22:33.67 -31:35:20.6
251.06712 3.13523 galactic Pup Second-epoch detections are separated by 2.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:22:33.67 -31:35:20.6 (user input) | T | P | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.5937,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.0937 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-02-26_22-21-45_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-04-Q2b1x1_214540_TTUQ2b1x1_17233_NjGh89UU/fd_Pup-04-Q2b1x1_2026-03-28_21-14-21_20.00sec_-10.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-04-Q2b1x1_214540_TTUQ2b1x1_17233_NjGh89UU/fd_Pup-04-Q2b1x1_2026-03-28_21-15-10_20.00sec_-10.00C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:22:33.67 -31:35:20.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-04-Q2b1x1_2026-02-26_22-21-45_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Pup-04-Q2b1x1_2026-03-28_21-15-10_20_00sec_-10_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-04-Q2b1x1_2026-02-26_22-21-45_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Pup-04-Q2b1x1_2026-03-28_21-14-21_20_00sec_-10_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-04-Q2b1x1_2026-02-26_22-21-45_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Pup-04-Q2b1x1_2026-03-28_21-15-10_20_00sec_-10_00C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-04-Q2b1x1_2026-02-26_22-21-45_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png resample_wcs_fd_Pup-04-Q2b1x1_2026-03-28_21-14-21_20_00sec_-10_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0881 2461128.5881 13.39 07:24:13.61 -31:52:58.5
244.93734 -7.64838 galactic CMa Second-epoch detections are separated by 1.2" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J111.0554-31.8847 | 07:24:13.61 -31:52:58.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 J111.0554-31.8847,2461128.5881,13.39,0.05,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
ATO J111.0554-31.8847 20260329.0881 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/Pup-03-Q2b1x1_2026-03-20_20-55-10_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-03-Q2b1x1_214339_TTUQ2b1x1_26869_erOrj41k/fd_Pup-03-Q2b1x1_2026-03-28_21-06-19_20.00sec_-10.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Pup-03-Q2b1x1_214339_TTUQ2b1x1_26869_erOrj41k/fd_Pup-03-Q2b1x1_2026-03-28_21-07-11_20.00sec_-10.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:24:13.61 -31:52:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-03-Q2b1x1_2026-03-20_20-55-10_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png resample_wcs_fd_Pup-03-Q2b1x1_2026-03-28_21-07-11_20_00sec_-10_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q2b1x1_2026-03-20_20-55-10_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png resample_wcs_fd_Pup-03-Q2b1x1_2026-03-28_21-06-19_20_00sec_-10_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_Pup-03-Q2b1x1_2026-03-20_20-55-10_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png resample_wcs_fd_Pup-03-Q2b1x1_2026-03-28_21-07-11_20_00sec_-10_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q2b1x1_2026-03-20_20-55-10_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png resample_wcs_fd_Pup-03-Q2b1x1_2026-03-28_21-06-19_20_00sec_-10_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.0975 2461128.5975 14.09 03:27:17.86 +43:44:35.5
150.46463 -10.64062 galactic Per Second-epoch detections are separated by 6.7" 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 | target | 03:27:17.86 +43:44:35.5 (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 29.0975* 03 27 17.86 +43 44 35.5 14.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.5975,14.09,0.05,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 20260329.0975 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/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Per-02-Q2b1x1_214935_TTUQ2b1x1_641_voP42cZt/fd_Per-02-Q2b1x1_2026-03-28_21-19-52_20.00sec_-10.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Per-02-Q2b1x1_214935_TTUQ2b1x1_641_voP42cZt/fd_Per-02-Q2b1x1_2026-03-28_21-20-44_20.00sec_-10.00C_LIGHT_0017.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:27:17.86 +43:44:35.5 ;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_Per-02-Q2b1x1_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png resample_wcs_fd_Per-02-Q2b1x1_2026-03-28_21-20-44_20_00sec_-10_00C_LIGHT_0017_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png resample_wcs_fd_Per-02-Q2b1x1_2026-03-28_21-19-52_20_00sec_-10_00C_LIGHT_0016_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png resample_wcs_fd_Per-02-Q2b1x1_2026-03-28_21-20-44_20_00sec_-10_00C_LIGHT_0017_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png resample_wcs_fd_Per-02-Q2b1x1_2026-03-28_21-19-52_20_00sec_-10_00C_LIGHT_0016_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1131 2461128.6131 13.90 03:45:00.19 +61:49:30.0
141.95149 5.54269 galactic Cam 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 486571729664118400 | 03:44:53.86 +61:49:27.2 (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 486571729664118400,2461128.6131,13.90,0.05,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 486571729664118400 20260329.1131 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/Cam-08-Q2b1x1_2026-01-20_20-04-43_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cam-08-Q2b1x1_214740_TTUQ2b1x1_796_GBydH8c3/fd_Cam-08-Q2b1x1_2026-03-28_21-42-19_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cam-08-Q2b1x1_214740_TTUQ2b1x1_796_GBydH8c3/fd_Cam-08-Q2b1x1_2026-03-28_21-43-01_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:00.19 +61:49:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Cam-08-Q2b1x1_2026-03-28_21-43-01_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Cam-08-Q2b1x1_2026-03-28_21-42-19_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Cam-08-Q2b1x1_2026-03-28_21-43-01_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q2b1x1_2026-01-20_20-04-43_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Cam-08-Q2b1x1_2026-03-28_21-42-19_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 29.0997* 04 10 19.73 +37 32 36.4 14.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.5997,14.60,0.05,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
target 20260329.0997 14.60CV 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/Per-05-Q2b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Per-05-Q2b1x1_215132_TTUQ2b1x1_18087_kP0srI97/fd_Per-05-Q2b1x1_2026-03-28_21-23-01_20.00sec_-10.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Per-05-Q2b1x1_215132_TTUQ2b1x1_18087_kP0srI97/fd_Per-05-Q2b1x1_2026-03-28_21-23-43_20.00sec_-10.00C_LIGHT_0021.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:19.73 +37:32:36.4 ;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_Per-05-Q2b1x1_2026-02-11_20-19-24_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-28_21-23-43_20_00sec_-10_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-28_21-23-01_20_00sec_-10_00C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-28_21-23-43_20_00sec_-10_00C_LIGHT_0021_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2026-02-11_20-19-24_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-28_21-23-01_20_00sec_-10_00C_LIGHT_0020_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1091 2461128.6091 12.62 05:40:37.44 +19:45:25.3
187.23944 -5.77193 galactic Tau Second-epoch detections are separated by 2.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.1513+19.7558 | 05:40:36.17 +19:45:33.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.378+/-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 29.1091* 05 40 37.44 +19 45 25.3 12.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.1513+19.7558,2461128.6091,12.62,0.05,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
ATO J085.1513+19.7558 20260329.1091 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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_215534_TTUQ2b1x1_6305_uduWIC7l/fd_Tau-04-Q2b1x1_2026-03-28_21-36-35_20.00sec_-10.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_215534_TTUQ2b1x1_6305_uduWIC7l/fd_Tau-04-Q2b1x1_2026-03-28_21-37-24_20.00sec_-10.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:40:37.44 +19:45:25.3 ;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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-24_20_00sec_-10_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-36-35_20_00sec_-10_00C_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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-24_20_00sec_-10_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-36-35_20_00sec_-10_00C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1091 2461128.6091 13.69 05:58:15.88 +25:59:12.3
183.96742 0.90789 galactic Tau Second-epoch detections are separated by 2.6" 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 J089.5793+25.9853 | 05:58:15.88 +25:59:12.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (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 29.1091* 05 58 15.88 +25 59 12.3 13.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.5793+25.9853,2461128.6091,13.69,0.05,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 J089.5793+25.9853 20260329.1091 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_215534_TTUQ2b1x1_6305_uduWIC7l/fd_Tau-04-Q2b1x1_2026-03-28_21-36-35_20.00sec_-10.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_215534_TTUQ2b1x1_6305_uduWIC7l/fd_Tau-04-Q2b1x1_2026-03-28_21-37-24_20.00sec_-10.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:15.88 +25:59:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-24_20_00sec_-10_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-36-35_20_00sec_-10_00C_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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-24_20_00sec_-10_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-36-35_20_00sec_-10_00C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1091 2461128.6091 14.03 05:38:25.83 +20:34:24.1
186.26948 -5.78102 galactic Tau Second-epoch detections are separated by 5.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3402686332724163328 | 05:38:26.86 +20:34:50.0 (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 29.1091* 05 38 25.83 +20 34 24.1 14.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3402686332724163328,2461128.6091,14.03,0.05,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 3402686332724163328 20260329.1091 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_215534_TTUQ2b1x1_6305_uduWIC7l/fd_Tau-04-Q2b1x1_2026-03-28_21-36-35_20.00sec_-10.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_215534_TTUQ2b1x1_6305_uduWIC7l/fd_Tau-04-Q2b1x1_2026-03-28_21-37-24_20.00sec_-10.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:25.83 +20:34:24.1 ;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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-24_20_00sec_-10_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-36-35_20_00sec_-10_00C_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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-24_20_00sec_-10_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-36-35_20_00sec_-10_00C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1079 2461128.6079 13.94 05:46:10.70 +08:19:17.5
197.87008 -10.45052 galactic Ori Second-epoch detections are separated by 6.7" 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 | target | 05:46:10.70 +08:19:17.5 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1079* 05 46 10.70 +08 19 17.5 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6079,13.94,0.05,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 20260329.1079 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/Ori-04-Q2b1x1_2026-02-21_20-50-02_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_215935_TTUQ2b1x1_5691_IcR6i3dD/fd_Ori-04-Q2b1x1_2026-03-28_21-34-47_20.00sec_-10.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_215935_TTUQ2b1x1_5691_IcR6i3dD/fd_Ori-04-Q2b1x1_2026-03-28_21-35-34_20.00sec_-10.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:10.70 +08:19:17.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-35-34_20_00sec_-10_00C_LIGHT_0037_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-47_20_00sec_-10_00C_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_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-35-34_20_00sec_-10_00C_LIGHT_0037_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-47_20_00sec_-10_00C_LIGHT_0036_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1079 2461128.6079 13.04 06:22:28.03 +07:06:38.8
203.29132 -3.14681 galactic Mon Second-epoch detections are separated by 0.6" 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 3324218551537975936 | 06:22:28.28 +07:06:06.9 (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 3324218551537975936,2461128.6079,13.04,0.05,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
Gaia DR3 3324218551537975936 20260329.1079 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/Ori-04-Q2b1x1_2026-02-21_20-50-02_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q2b1x1_2026-02-21_20-50-52_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_215935_TTUQ2b1x1_5691_IcR6i3dD/fd_Ori-04-Q2b1x1_2026-03-28_21-34-47_20.00sec_-10.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-04-Q2b1x1_215935_TTUQ2b1x1_5691_IcR6i3dD/fd_Ori-04-Q2b1x1_2026-03-28_21-35-34_20.00sec_-10.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:28.03 +07:06:38.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-35-34_20_00sec_-10_00C_LIGHT_0037_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-47_20_00sec_-10_00C_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_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-35-34_20_00sec_-10_00C_LIGHT_0037_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q2b1x1_2026-02-21_20-50-02_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Ori-04-Q2b1x1_2026-03-28_21-34-47_20_00sec_-10_00C_LIGHT_0036_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 10.48 01:57:42.59 +42:42:36.6
135.69751 -18.51288 galactic And Second-epoch detections are separated by 0.8" 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 346134133102034560 | 01:57:42.56 +42:42:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.703+/-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!
TCP 2026 03 29.1283* 01 57 42.59 +42 42 36.6 10.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 346134133102034560,2461128.6283,10.48,0.05,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
Gaia DR3 346134133102034560 20260329.1283 10.48CV 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/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:57:42.59 +42:42:36.6 ;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_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 12.51 01:54:00.39 +42:23:43.3
135.08884 -18.99461 galactic And Second-epoch detections are separated by 1.1" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 346070292707639168 | 01:54:00.17 +42:23:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 01 54 00.39 +42 23 43.3 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 346070292707639168,2461128.6283,12.51,0.05,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
Gaia DR3 346070292707639168 20260329.1283 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/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:54:00.39 +42:23:43.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 11.12 01:54:08.84 +43:55:05.0
134.70939 -17.51494 galactic And Second-epoch detections are separated by 0.3" 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 349663256189068544 | 01:54:08.73 +43:55:05.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.298+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 01 54 08.84 +43 55 05.0 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 349663256189068544,2461128.6283,11.12,0.05,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 349663256189068544 20260329.1283 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/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:54:08.84 +43:55:05.0 ;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_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 12.82 02:00:13.38 +41:52:06.0
136.41294 -19.19576 galactic And Second-epoch detections are separated by 0.5" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J030.0567+41.8668 | 02:00:13.38 +41:52:06.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.661+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 02 00 13.38 +41 52 06.0 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J030.0567+41.8668,2461128.6283,12.82,0.05,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
ATO J030.0567+41.8668 20260329.1283 12.82CV 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/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:00:13.38 +41:52:06.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 13.19 01:55:44.55 +42:24:42.0
135.41184 -18.89645 galactic And Second-epoch detections are separated by 4.2" 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 | 01:55:44.55 +42:24:42.0 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 01 55 44.55 +42 24 42.0 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6283,13.19,0.05,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
target 20260329.1283 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/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:44.55 +42:24:42.0 ;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_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 12.45 02:06:06.87 +41:52:17.0
137.52241 -18.87491 galactic And Second-epoch detections are separated by 0.9" 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 | ATO J031.5157+41.8682 | 02:06:06.76 +41:52:17.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 02 06 06.87 +41 52 17.0 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J031.5157+41.8682,2461128.6283,12.45,0.05,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
ATO J031.5157+41.8682 20260329.1283 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:06.87 +41:52:17.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 12.68 01:52:29.94 +42:57:02.3
134.65865 -18.52643 galactic And Second-epoch detections are separated by 0.3" 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 349098927549384192 | 01:52:29.78 +42:57:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.223+/-0.030 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 01 52 29.94 +42 57 02.3 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 349098927549384192,2461128.6283,12.68,0.05,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
Gaia DR3 349098927549384192 20260329.1283 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:52:29.94 +42:57:02.3 ;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_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 12.81 01:50:16.05 +44:05:34.1
133.95521 -17.51613 galactic And Second-epoch detections are separated by 3.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 349504612980163840 | 01:50:15.92 +44:05:36.2 (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!
TCP 2026 03 29.1283* 01 50 16.05 +44 05 34.1 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 349504612980163840,2461128.6283,12.81,0.05,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
Gaia DR3 349504612980163840 20260329.1283 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/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:50:16.05 +44:05:34.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 12.46 01:56:07.54 +41:48:46.4
135.65036 -19.45576 galactic And Second-epoch detections are separated by 1.5" 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 | ATO J029.0310+41.8135 | 01:56:07.46 +41:48:48.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.284+/-0.026 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 01 56 07.54 +41 48 46.4 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J029.0310+41.8135,2461128.6283,12.46,0.05,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
ATO J029.0310+41.8135 20260329.1283 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/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:56:07.54 +41:48:46.4 ;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_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 12.80 01:53:44.55 +44:52:38.6
134.38451 -16.60440 galactic And Second-epoch detections are separated by 2.0" 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 349730395117657600 | 01:53:44.23 +44:52:38.9 (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 29.1283* 01 53 44.55 +44 52 38.6 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 349730395117657600,2461128.6283,12.80,0.05,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
Gaia DR3 349730395117657600 20260329.1283 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:44.55 +44:52:38.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 13.11 02:03:42.59 +41:53:35.2
137.06371 -18.98687 galactic And Second-epoch detections are separated by 1.7" 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 | target | 02:03:42.59 +41:53:35.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 02 03 42.59 +41 53 35.2 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6283,13.11,0.05,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
target 20260329.1283 13.11CV 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/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:42.59 +41:53:35.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 11.55 01:55:48.21 +42:23:44.7
135.42772 -18.90888 galactic And Second-epoch detections are separated by 0.8" 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 346148907789415168 | 01:55:48.18 +42:23:46.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.244+/-0.030 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 01 55 48.21 +42 23 44.7 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 346148907789415168,2461128.6283,11.55,0.05,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 346148907789415168 20260329.1283 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:48.21 +42:23:44.7 ;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_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 11.84 01:56:36.66 +43:04:00.4
135.39336 -18.22243 galactic And Second-epoch detections are separated by 0.4" 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 346205631419516800 | 01:56:36.51 +43:04:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.011+/-0.040 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 01 56 36.66 +43 04 00.4 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 346205631419516800,2461128.6283,11.84,0.05,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 346205631419516800 20260329.1283 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:56:36.66 +43:04:00.4 ;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_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 12.44 01:49:14.79 +45:09:51.2
133.50799 -16.51710 galactic And Second-epoch detections are separated by 0.6" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J027.3111+45.1614 | 01:49:14.71 +45:09:53.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 01 49 14.79 +45 09 51.2 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J027.3111+45.1614,2461128.6283,12.44,0.05,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 J027.3111+45.1614 20260329.1283 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:49:14.79 +45:09:51.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1283 2461128.6283 12.19 01:55:17.38 +42:20:37.8
135.34508 -18.98367 galactic And Second-epoch detections are separated by 0.9" 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 J028.8273+42.3429 | 01:55:17.26 +42:20:40.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1283* 01 55 17.38 +42 20 37.8 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J028.8273+42.3429,2461128.6283,12.19,0.05,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
ATO J028.8273+42.3429 20260329.1283 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-03-26_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2026-01-08_22-04-20_20.00sec_-14.90C_LIGHT_0134.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-04-13_20.00sec_-15.00C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_And-03-Q2b1x1_221138_TTUQ2b1x1_3787_zcMQbi87/fd_And-03-Q2b1x1_2026-03-28_22-05-04_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:17.38 +42:20:37.8 ;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_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-05-04_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2026-01-08_22-03-26_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png resample_wcs_fd_And-03-Q2b1x1_2026-03-28_22-04-13_20_00sec_-15_00C_LIGHT_0069_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1375 2461128.6375 11.67 03:32:59.41 +27:49:07.4
161.35252 -22.75181 galactic Tau Second-epoch detections are separated by 1.0" 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 J053.2558+27.8162 | 03:32:59.38 +27:49:08.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.659+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1375* 03 32 59.41 +27 49 07.4 11.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J053.2558+27.8162,2461128.6375,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J053.2558+27.8162 20260329.1375 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:59.41 +27:49:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1375 2461128.6375 11.38 03:32:34.10 +28:00:57.7
161.14007 -22.65589 galactic Tau Second-epoch detections are separated by 1.2" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 119442735560772736 | 03:32:34.04 +28:00:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.348+/-0.027 (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 29.1375* 03 32 34.10 +28 00 57.7 11.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 119442735560772736,2461128.6375,11.38,0.05,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 119442735560772736 20260329.1375 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:34.10 +28:00:57.7 ;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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1329 2461128.6329 12.97 02:47:39.18 +34:52:37.5
148.41454 -22.17972 galactic Per Second-epoch detections are separated by 0.5" 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 | target | 02:47:39.18 +34:52:37.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.638+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1330* 02 47 39.18 +34 52 37.5 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6329,12.97,0.05,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 20260329.1329 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Per-04-Q2b1x1_221535_TTUQ2b1x1_6543_RjDU7N04/fd_Per-04-Q2b1x1_2026-03-28_22-10-55_20.00sec_-15.00C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Per-04-Q2b1x1_221535_TTUQ2b1x1_6543_RjDU7N04/fd_Per-04-Q2b1x1_2026-03-28_22-11-37_20.00sec_-15.00C_LIGHT_0078.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:47:39.18 +34:52:37.5 ;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_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-28_22-11-37_20_00sec_-15_00C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-28_22-10-55_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-28_22-11-37_20_00sec_-15_00C_LIGHT_0078_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-28_22-10-55_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1319 2461128.6319 13.04 03:16:42.53 +20:44:00.5
162.99321 -30.61282 galactic Ari Second-epoch detections are separated by 1.9" 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 | 03:16:42.53 +20:44:00.5 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.368+/-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 29.1319* 03 16 42.53 +20 44 00.5 13.0 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6319,13.04,0.05,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 20260329.1319 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/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-02-Q2b1x1_222336_TTUQ2b1x1_3384_5GXHCeaG/fd_Tau-02-Q2b1x1_2026-03-28_22-09-25_20.00sec_-14.90C_LIGHT_0075.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-02-Q2b1x1_222336_TTUQ2b1x1_3384_5GXHCeaG/fd_Tau-02-Q2b1x1_2026-03-28_22-10-08_20.00sec_-15.00C_LIGHT_0076.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:42.53 +20:44:00.5 ;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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-10-08_20_00sec_-15_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-09-25_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-10-08_20_00sec_-15_00C_LIGHT_0076_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-09-25_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1319 2461128.6319 13.01 03:26:42.60 +18:12:31.1
166.97975 -31.07889 galactic Tau Second-epoch detections are separated by 1.0" 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 | target | 03:26:42.60 +18:12:31.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.591+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1319* 03 26 42.60 +18 12 31.1 13.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6319,13.01,0.05,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
target 20260329.1319 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-02-Q2b1x1_222336_TTUQ2b1x1_3384_5GXHCeaG/fd_Tau-02-Q2b1x1_2026-03-28_22-09-25_20.00sec_-14.90C_LIGHT_0075.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-02-Q2b1x1_222336_TTUQ2b1x1_3384_5GXHCeaG/fd_Tau-02-Q2b1x1_2026-03-28_22-10-08_20.00sec_-15.00C_LIGHT_0076.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:26:42.60 +18:12:31.1 ;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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-10-08_20_00sec_-15_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-09-25_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-10-08_20_00sec_-15_00C_LIGHT_0076_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-09-25_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1319 2461128.6319 13.31 03:25:35.03 +18:52:40.8
166.23711 -30.74226 galactic Tau 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 | target | 03:25:35.03 +18:52:40.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.460+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1319* 03 25 35.03 +18 52 40.8 13.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6319,13.31,0.05,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 20260329.1319 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/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-02-Q2b1x1_222336_TTUQ2b1x1_3384_5GXHCeaG/fd_Tau-02-Q2b1x1_2026-03-28_22-09-25_20.00sec_-14.90C_LIGHT_0075.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-02-Q2b1x1_222336_TTUQ2b1x1_3384_5GXHCeaG/fd_Tau-02-Q2b1x1_2026-03-28_22-10-08_20.00sec_-15.00C_LIGHT_0076.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:35.03 +18:52:40.8 ;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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-10-08_20_00sec_-15_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-09-25_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-10-08_20_00sec_-15_00C_LIGHT_0076_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-28_22-09-25_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1262 2461128.6262 13.93 05:57:43.10 +28:03:29.2
182.11195 1.83772 galactic Tau Second-epoch detections are separated by 1.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3431276040231115008 | 05:57:42.88 +28:03:12.8 (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!
TCP 2026 03 29.1262* 05 57 43.10 +28 03 29.2 13.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3431276040231115008,2461128.6262,13.93,0.05,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
Gaia DR3 3431276040231115008 20260329.1262 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/Aur-06-Q2b1x1_2026-02-10_21-15-02_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-06-Q2b1x1_222137_TTUQ2b1x1_12521_TPaZ41Wt/fd_Aur-06-Q2b1x1_2026-03-28_22-01-07_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-06-Q2b1x1_222137_TTUQ2b1x1_12521_TPaZ41Wt/fd_Aur-06-Q2b1x1_2026-03-28_22-01-56_20.00sec_-15.00C_LIGHT_0066.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:43.10 +28:03:29.2 ;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_Aur-06-Q2b1x1_2026-02-10_21-15-02_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png resample_wcs_fd_Aur-06-Q2b1x1_2026-03-28_22-01-56_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-06-Q2b1x1_2026-02-10_21-15-02_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png resample_wcs_fd_Aur-06-Q2b1x1_2026-03-28_22-01-07_20_00sec_-15_00C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-06-Q2b1x1_2026-02-10_21-15-02_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png resample_wcs_fd_Aur-06-Q2b1x1_2026-03-28_22-01-56_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-06-Q2b1x1_2026-02-10_21-15-02_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png resample_wcs_fd_Aur-06-Q2b1x1_2026-03-28_22-01-07_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1262 2461128.6262 10.83 05:52:21.42 +32:33:54.2
177.63138 3.10766 galactic Aur Second-epoch detections are separated by 1.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.0714+32.5633 | 05:52:20.31 +32:33:49.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3 1954StoAn..18a...1L NGC 2099 84
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.0714+32.5633,2461128.6262,10.83,0.05,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
ATO J088.0714+32.5633 20260329.1262 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-10_21-15-02_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-06-Q2b1x1_222137_TTUQ2b1x1_12521_TPaZ41Wt/fd_Aur-06-Q2b1x1_2026-03-28_22-01-07_20.00sec_-15.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-06-Q2b1x1_222137_TTUQ2b1x1_12521_TPaZ41Wt/fd_Aur-06-Q2b1x1_2026-03-28_22-01-56_20.00sec_-15.00C_LIGHT_0066.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:21.42 +32:33:54.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-06-Q2b1x1_2026-02-10_21-15-02_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png resample_wcs_fd_Aur-06-Q2b1x1_2026-03-28_22-01-56_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-06-Q2b1x1_2026-02-10_21-15-02_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png resample_wcs_fd_Aur-06-Q2b1x1_2026-03-28_22-01-07_20_00sec_-15_00C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-06-Q2b1x1_2026-02-10_21-15-02_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png resample_wcs_fd_Aur-06-Q2b1x1_2026-03-28_22-01-56_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-06-Q2b1x1_2026-02-10_21-15-02_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png resample_wcs_fd_Aur-06-Q2b1x1_2026-03-28_22-01-07_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1243 2461128.6243 11.14 05:28:05.30 +35:19:31.8
172.61945 0.30738 galactic Aur Second-epoch detections are separated by 7.6" 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 | ATO J082.0215+35.3205 | 05:28:06.64 +35:19:14.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: em: 1956BOTT....2n..19G GGA 337
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.0215+35.3205,2461128.6243,11.14,0.05,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 J082.0215+35.3205 20260329.1243 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-03-Q2b1x1_221735_TTUQ2b1x1_29990_NzooqWiW/fd_Aur-03-Q2b1x1_2026-03-28_21-58-23_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-03-Q2b1x1_221735_TTUQ2b1x1_29990_NzooqWiW/fd_Aur-03-Q2b1x1_2026-03-28_21-59-06_20.00sec_-15.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:05.30 +35:19:31.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-59-06_20_00sec_-15_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-58-23_20_00sec_-15_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-59-06_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-58-23_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1243 2461128.6243 13.37 06:00:10.12 +41:21:37.4
170.71440 8.80781 galactic Aur Second-epoch detections are separated by 4.9" 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 | target | 06:00:10.12 +41:21:37.4 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.622+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6243,13.37,0.05,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 20260329.1243 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-03-Q2b1x1_221735_TTUQ2b1x1_29990_NzooqWiW/fd_Aur-03-Q2b1x1_2026-03-28_21-58-23_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-03-Q2b1x1_221735_TTUQ2b1x1_29990_NzooqWiW/fd_Aur-03-Q2b1x1_2026-03-28_21-59-06_20.00sec_-15.00C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:10.12 +41:21:37.4 ;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_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-59-06_20_00sec_-15_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-58-23_20_00sec_-15_00C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-59-06_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-58-23_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1101* 05 48 40.63 +18 15 22.7 13.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6101,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1101 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_222736_TTUQ2b1x1_18146_Zs22AYLu/fd_Tau-04-Q2b1x1_2026-03-28_21-37-56_20.00sec_-10.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_222736_TTUQ2b1x1_18146_Zs22AYLu/fd_Tau-04-Q2b1x1_2026-03-28_21-38-41_20.00sec_-9.90C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:40.63 +18:15:22.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-38-41_20_00sec_-9_90C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-56_20_00sec_-10_00C_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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-38-41_20_00sec_-9_90C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-56_20_00sec_-10_00C_LIGHT_0040_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1101 2461128.6101 13.76 05:47:21.11 +23:52:59.4
184.52130 -2.29168 galactic Tau Second-epoch detections are separated by 1.5" 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 | ATO J086.8387+23.8837 | 05:47:21.11 +23:52:59.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1101* 05 47 21.11 +23 52 59.4 13.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.8387+23.8837,2461128.6101,13.76,0.05,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
ATO J086.8387+23.8837 20260329.1101 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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_222736_TTUQ2b1x1_18146_Zs22AYLu/fd_Tau-04-Q2b1x1_2026-03-28_21-37-56_20.00sec_-10.00C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-04-Q2b1x1_222736_TTUQ2b1x1_18146_Zs22AYLu/fd_Tau-04-Q2b1x1_2026-03-28_21-38-41_20.00sec_-9.90C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:21.11 +23:52:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-38-41_20_00sec_-9_90C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-56_20_00sec_-10_00C_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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-38-41_20_00sec_-9_90C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-28_21-37-56_20_00sec_-10_00C_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,2461128.6297,13.18,0.05,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
target 20260329.1297 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-05-Q2b1x1_2025-12-22_23-54-22_20.00sec_-14.90C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Eri-05-Q2b1x1_224336_TTUQ2b1x1_30589_NSTJACr0/fd_Eri-05-Q2b1x1_2026-03-28_22-06-11_20.00sec_-14.90C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Eri-05-Q2b1x1_224336_TTUQ2b1x1_30589_NSTJACr0/fd_Eri-05-Q2b1x1_2026-03-28_22-06-55_20.00sec_-14.90C_LIGHT_0072.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:34.74 -11:29:52.7 ;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_Eri-05-Q2b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q2b1x1_2026-03-28_22-06-55_20_00sec_-14_90C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-05-Q2b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q2b1x1_2026-03-28_22-06-11_20_00sec_-14_90C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-05-Q2b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q2b1x1_2026-03-28_22-06-55_20_00sec_-14_90C_LIGHT_0072_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-05-Q2b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q2b1x1_2026-03-28_22-06-11_20_00sec_-14_90C_LIGHT_0071_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1297 2461128.6297 12.79 04:46:17.67 -13:46:00.5
211.67565 -33.87698 galactic Eri Second-epoch detections are separated by 0.9" and 1.1 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 | 04:46:17.67 -13:46:00.5 (user input) | T | P | (position from user input) J-Ks=0.707+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1297* 04 46 17.67 -13 46 00.5 12.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6297,12.79,0.05,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 20260329.1297 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-05-Q2b1x1_2025-12-22_23-54-22_20.00sec_-14.90C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-05-Q2b1x1_2025-12-22_23-55-03_20.00sec_-15.00C_LIGHT_0273.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Eri-05-Q2b1x1_224336_TTUQ2b1x1_30589_NSTJACr0/fd_Eri-05-Q2b1x1_2026-03-28_22-06-11_20.00sec_-14.90C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Eri-05-Q2b1x1_224336_TTUQ2b1x1_30589_NSTJACr0/fd_Eri-05-Q2b1x1_2026-03-28_22-06-55_20.00sec_-14.90C_LIGHT_0072.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:17.67 -13:46:00.5 ;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_Eri-05-Q2b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q2b1x1_2026-03-28_22-06-55_20_00sec_-14_90C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-05-Q2b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q2b1x1_2026-03-28_22-06-11_20_00sec_-14_90C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-05-Q2b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q2b1x1_2026-03-28_22-06-55_20_00sec_-14_90C_LIGHT_0072_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-05-Q2b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q2b1x1_2026-03-28_22-06-11_20_00sec_-14_90C_LIGHT_0071_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1421 2461128.6420 13.73 06:18:40.89 -03:05:52.2
211.96043 -8.69805 galactic Ori Second-epoch detections are separated by 3.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3117656325686342656 | 06:18:41.80 -03:05:11.8 (Gaia DR3) | RS (local) | (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!
TCP 2026 03 29.1421* 06 18 40.89 -03 05 52.2 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3117656325686342656,2461128.6420,13.73,0.05,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
Gaia DR3 3117656325686342656 20260329.1421 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/Ori-06-Q2b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-06-Q2b1x1_224137_TTUQ2b1x1_16622_Z8B2z0qM/fd_Ori-06-Q2b1x1_2026-03-28_22-24-01_20.00sec_-15.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-06-Q2b1x1_224137_TTUQ2b1x1_16622_Z8B2z0qM/fd_Ori-06-Q2b1x1_2026-03-28_22-24-45_20.00sec_-15.00C_LIGHT_0094.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:40.89 -03:05:52.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-06-Q2b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q2b1x1_2026-03-28_22-24-45_20_00sec_-15_00C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-06-Q2b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q2b1x1_2026-03-28_22-24-01_20_00sec_-15_00C_LIGHT_0093_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q2b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q2b1x1_2026-03-28_22-24-45_20_00sec_-15_00C_LIGHT_0094_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q2b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q2b1x1_2026-03-28_22-24-01_20_00sec_-15_00C_LIGHT_0093_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1421* 05 41 27.13 -01 53 31.9 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6420,13.76,0.05,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 20260329.1421 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/Ori-06-Q2b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-06-Q2b1x1_224137_TTUQ2b1x1_16622_Z8B2z0qM/fd_Ori-06-Q2b1x1_2026-03-28_22-24-01_20.00sec_-15.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-06-Q2b1x1_224137_TTUQ2b1x1_16622_Z8B2z0qM/fd_Ori-06-Q2b1x1_2026-03-28_22-24-45_20.00sec_-15.00C_LIGHT_0094.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:27.13 -01:53:31.9 ;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_Ori-06-Q2b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q2b1x1_2026-03-28_22-24-45_20_00sec_-15_00C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-06-Q2b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q2b1x1_2026-03-28_22-24-01_20_00sec_-15_00C_LIGHT_0093_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q2b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q2b1x1_2026-03-28_22-24-45_20_00sec_-15_00C_LIGHT_0094_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q2b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q2b1x1_2026-03-28_22-24-01_20_00sec_-15_00C_LIGHT_0093_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1385 2461128.6385 13.95 06:16:51.55 -10:52:47.5
218.85239 -12.55834 galactic Mon Second-epoch detections are separated by 0.9" 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 J094.2145-10.8802 | 06:16:51.55 -10:52:47.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.404+/-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
ATO J094.2145-10.8802,2461128.6385,13.95,0.05,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
ATO J094.2145-10.8802 20260329.1385 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/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Mon-04-Q2b1x1_224536_TTUQ2b1x1_4405_bhX1OooR/fd_Mon-04-Q2b1x1_2026-03-28_22-18-57_20.00sec_-14.90C_LIGHT_0087.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Mon-04-Q2b1x1_224536_TTUQ2b1x1_4405_bhX1OooR/fd_Mon-04-Q2b1x1_2026-03-28_22-19-43_20.00sec_-15.00C_LIGHT_0088.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:51.55 -10:52:47.5 ;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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-28_22-19-43_20_00sec_-15_00C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-28_22-18-57_20_00sec_-14_90C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-28_22-19-43_20_00sec_-15_00C_LIGHT_0088_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-28_22-18-57_20_00sec_-14_90C_LIGHT_0087_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6543,14.35,0.05,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 20260329.1543 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cam-06-Q2b1x1_225742_TTUQ2b1x1_29003_tGfqBW7c/fd_Cam-06-Q2b1x1_2026-03-28_22-41-43_20.00sec_-14.90C_LIGHT_0109.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cam-06-Q2b1x1_225742_TTUQ2b1x1_29003_tGfqBW7c/fd_Cam-06-Q2b1x1_2026-03-28_22-42-26_20.00sec_-14.90C_LIGHT_0110.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:21:48.80 +69:32:38.0 ;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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-28_22-42-26_20_00sec_-14_90C_LIGHT_0110_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-28_22-41-43_20_00sec_-14_90C_LIGHT_0109_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-28_22-42-26_20_00sec_-14_90C_LIGHT_0110_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-28_22-41-43_20_00sec_-14_90C_LIGHT_0109_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6251,14.27,0.05,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
target 20260329.1251 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-03-Q2b1x1_231738_TTUQ2b1x1_29175_K7u3QekW/fd_Aur-03-Q2b1x1_2026-03-28_21-59-38_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-03-Q2b1x1_231738_TTUQ2b1x1_29175_K7u3QekW/fd_Aur-03-Q2b1x1_2026-03-28_22-00-22_20.00sec_-14.90C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:51.25 +37:30:43.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_22-00-22_20_00sec_-14_90C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-59-38_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_22-00-22_20_00sec_-14_90C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-59-38_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1251 2461128.6251 13.46 06:01:43.24 +40:48:43.6
171.34319 8.80321 galactic Aur Second-epoch detections are separated by 0.9" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:01:43.24 +40:48:43.6 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.198+/-0.037 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6251,13.46,0.05,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 20260329.1251 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/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-03-Q2b1x1_231738_TTUQ2b1x1_29175_K7u3QekW/fd_Aur-03-Q2b1x1_2026-03-28_21-59-38_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-03-Q2b1x1_231738_TTUQ2b1x1_29175_K7u3QekW/fd_Aur-03-Q2b1x1_2026-03-28_22-00-22_20.00sec_-14.90C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:43.24 +40:48:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_22-00-22_20_00sec_-14_90C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-59-38_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_22-00-22_20_00sec_-14_90C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-28_21-59-38_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6744,14.47,0.05,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 20260329.1744 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/Cam-05-Q2b1x1_2026-03-20_02-59-56_20.00sec_-14.90C_LIGHT_0361.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cam-05-Q2b1x1_233932_TTUQ2b1x1_21735_eWvMDgA6/fd_Cam-05-Q2b1x1_2026-03-28_23-10-35_20.00sec_-14.90C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Cam-05-Q2b1x1_233932_TTUQ2b1x1_21735_eWvMDgA6/fd_Cam-05-Q2b1x1_2026-03-28_23-11-22_20.00sec_-15.00C_LIGHT_0136.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:07:25.79 +77:59:46.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-05-Q2b1x1_2026-03-20_02-59-56_20_00sec_-14_90C_LIGHT_0361_fits__*pix.png resample_wcs_fd_Cam-05-Q2b1x1_2026-03-28_23-11-22_20_00sec_-15_00C_LIGHT_0136_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-05-Q2b1x1_2026-03-20_02-59-56_20_00sec_-14_90C_LIGHT_0361_fits__*pix.png resample_wcs_fd_Cam-05-Q2b1x1_2026-03-28_23-10-35_20_00sec_-14_90C_LIGHT_0135_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-05-Q2b1x1_2026-03-20_02-59-56_20_00sec_-14_90C_LIGHT_0361_fits__*pix.png resample_wcs_fd_Cam-05-Q2b1x1_2026-03-28_23-11-22_20_00sec_-15_00C_LIGHT_0136_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-05-Q2b1x1_2026-03-20_02-59-56_20_00sec_-14_90C_LIGHT_0361_fits__*pix.png resample_wcs_fd_Cam-05-Q2b1x1_2026-03-28_23-10-35_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1913 2461128.6913 13.37 12:14:57.39 +63:47:13.5
129.59218 52.86686 galactic Dra Second-epoch detections are separated by 8.8" and 4.0 pix This object is listed in asassn_transients_list.txt 5.8" SN 2026fvx 2026-03-21.12 15.6
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 | 12:14:57.39 +63:47:13.5 (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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6913,13.37,0.05,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 20260329.1913 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-04-Q2b1x1_2026-01-21_05-14-22_20.00sec_-15.00C_LIGHT_0545.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_UMa-04-Q2b1x1_235337_TTUQ2b1x1_27665_vhBRDKis/fd_UMa-04-Q2b1x1_2026-03-28_23-34-47_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_UMa-04-Q2b1x1_235337_TTUQ2b1x1_27665_vhBRDKis/fd_UMa-04-Q2b1x1_2026-03-28_23-35-42_20.00sec_-14.90C_LIGHT_0156.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:14:57.39 +63:47:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-04-Q2b1x1_2026-01-21_05-14-22_20_00sec_-15_00C_LIGHT_0545_fits__*pix.png resample_wcs_fd_UMa-04-Q2b1x1_2026-03-28_23-35-42_20_00sec_-14_90C_LIGHT_0156_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-04-Q2b1x1_2026-01-21_05-14-22_20_00sec_-15_00C_LIGHT_0545_fits__*pix.png resample_wcs_fd_UMa-04-Q2b1x1_2026-03-28_23-34-47_20_00sec_-14_90C_LIGHT_0155_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-04-Q2b1x1_2026-01-21_05-14-22_20_00sec_-15_00C_LIGHT_0545_fits__*pix.png resample_wcs_fd_UMa-04-Q2b1x1_2026-03-28_23-35-42_20_00sec_-14_90C_LIGHT_0156_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-04-Q2b1x1_2026-01-21_05-14-22_20_00sec_-15_00C_LIGHT_0545_fits__*pix.png resample_wcs_fd_UMa-04-Q2b1x1_2026-03-28_23-34-47_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png animation_v2.gif