Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 26.1924* 13 08 07.00 -14 17 37.2 13.6 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.6924,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.1924 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-13-Q2b1x1_235508_TTUQ2b1x1_28200_73pfz9fI/fd_Vir-13-Q2b1x1_2026-03-25_23-36-32_20.00sec_-10.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-13-Q2b1x1_235508_TTUQ2b1x1_28200_73pfz9fI/fd_Vir-13-Q2b1x1_2026-03-25_23-37-18_20.00sec_-10.00C_LIGHT_0409.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:08:07.00 -14:17:37.2 ;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_Vir-13-Q2b1x1_2026-02-27_03-51-10_20_00sec_-14_90C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-25_23-37-18_20_00sec_-10_00C_LIGHT_0409_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20_00sec_-14_90C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-25_23-36-32_20_00sec_-10_00C_LIGHT_0408_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20_00sec_-14_90C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-25_23-37-18_20_00sec_-10_00C_LIGHT_0409_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20_00sec_-14_90C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-25_23-36-32_20_00sec_-10_00C_LIGHT_0408_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.1961 2461125.6961 14.98 11:08:00.68 +46:51:03.5
161.90419 61.69096 galactic UMa Second-epoch detections are separated by 0.8" 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 | 11:08:00.68 +46:51:03.5 (user input) | T | P | (position from user input) J-Ks=1.665+/- (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!
TCP 2026 03 26.1961* 11 08 00.68 +46 51 03.5 15.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.6961,14.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.1961 14.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q2b1x1_2026-02-12_01-52-29_20.00sec_-14.90C_LIGHT_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_UMa-10-Q2b1x1_235911_TTUQ2b1x1_23978_NrQDhNII/fd_UMa-10-Q2b1x1_2026-03-25_23-41-46_20.00sec_-10.00C_LIGHT_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_UMa-10-Q2b1x1_235911_TTUQ2b1x1_23978_NrQDhNII/fd_UMa-10-Q2b1x1_2026-03-25_23-42-31_20.00sec_-10.00C_LIGHT_0415.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:08:00.68 +46:51:03.5 ;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-10-Q2b1x1_2026-02-12_01-52-29_20_00sec_-14_90C_LIGHT_0352_fits__*pix.png resample_wcs_fd_UMa-10-Q2b1x1_2026-03-25_23-42-31_20_00sec_-10_00C_LIGHT_0415_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-10-Q2b1x1_2026-02-12_01-52-29_20_00sec_-14_90C_LIGHT_0352_fits__*pix.png resample_wcs_fd_UMa-10-Q2b1x1_2026-03-25_23-41-46_20_00sec_-10_00C_LIGHT_0414_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-10-Q2b1x1_2026-02-12_01-52-29_20_00sec_-14_90C_LIGHT_0352_fits__*pix.png resample_wcs_fd_UMa-10-Q2b1x1_2026-03-25_23-42-31_20_00sec_-10_00C_LIGHT_0415_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-10-Q2b1x1_2026-02-12_01-52-29_20_00sec_-14_90C_LIGHT_0352_fits__*pix.png resample_wcs_fd_UMa-10-Q2b1x1_2026-03-25_23-41-46_20_00sec_-10_00C_LIGHT_0414_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2047 2461125.7047 14.38 11:43:02.88 +26:16:33.5
212.23754 74.71388 galactic Leo Second-epoch detections are separated by 4.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J175.7622+26.2767 | 11:43:02.88 +26:16:33.5 (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!
TCP 2026 03 26.2047* 11 43 02.88 +26 16 33.5 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J175.7622+26.2767,2461125.7047,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J175.7622+26.2767 20260326.2047 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_UMa-14-Q2b1x1_000103_TTUQ2b1x1_11832_Tn5JVGk5/fd_UMa-14-Q2b1x1_2026-03-25_23-54-14_20.00sec_-10.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_UMa-14-Q2b1x1_000103_TTUQ2b1x1_11832_Tn5JVGk5/fd_UMa-14-Q2b1x1_2026-03-25_23-55-01_20.00sec_-10.00C_LIGHT_0427.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:43:02.88 +26:16:33.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20_00sec_-14_90C_LIGHT_0096_fits__*pix.png resample_wcs_fd_UMa-14-Q2b1x1_2026-03-25_23-55-01_20_00sec_-10_00C_LIGHT_0427_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20_00sec_-14_90C_LIGHT_0096_fits__*pix.png resample_wcs_fd_UMa-14-Q2b1x1_2026-03-25_23-54-14_20_00sec_-10_00C_LIGHT_0426_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20_00sec_-14_90C_LIGHT_0096_fits__*pix.png resample_wcs_fd_UMa-14-Q2b1x1_2026-03-25_23-55-01_20_00sec_-10_00C_LIGHT_0427_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20_00sec_-14_90C_LIGHT_0096_fits__*pix.png resample_wcs_fd_UMa-14-Q2b1x1_2026-03-25_23-54-14_20_00sec_-10_00C_LIGHT_0426_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 26.2036* 12 31 39.39 +03 56 19.3 13.8 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7036,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2036 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q2b1x1_2026-02-27_03-04-45_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-03-Q2b1x1_000302_TTUQ2b1x1_487_aiK7EhNm/fd_Vir-03-Q2b1x1_2026-03-25_23-52-41_20.00sec_-10.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-03-Q2b1x1_000302_TTUQ2b1x1_487_aiK7EhNm/fd_Vir-03-Q2b1x1_2026-03-25_23-53-25_20.00sec_-10.00C_LIGHT_0425.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:31:39.39 +03:56:19.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-03-Q2b1x1_2026-02-27_03-04-45_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png resample_wcs_fd_Vir-03-Q2b1x1_2026-03-25_23-53-25_20_00sec_-10_00C_LIGHT_0425_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-03-Q2b1x1_2026-02-27_03-04-45_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png resample_wcs_fd_Vir-03-Q2b1x1_2026-03-25_23-52-41_20_00sec_-10_00C_LIGHT_0424_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-03-Q2b1x1_2026-02-27_03-04-45_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png resample_wcs_fd_Vir-03-Q2b1x1_2026-03-25_23-53-25_20_00sec_-10_00C_LIGHT_0425_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-03-Q2b1x1_2026-02-27_03-04-45_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png resample_wcs_fd_Vir-03-Q2b1x1_2026-03-25_23-52-41_20_00sec_-10_00C_LIGHT_0424_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,2461125.7189,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2189 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Dra-02-Q2b1x1_001700_TTUQ2b1x1_16843_FNs185b9/fd_Dra-02-Q2b1x1_2026-03-26_00-14-41_20.00sec_-10.00C_LIGHT_0440.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Dra-02-Q2b1x1_001700_TTUQ2b1x1_16843_FNs185b9/fd_Dra-02-Q2b1x1_2026-03-26_00-15-32_20.00sec_-9.90C_LIGHT_0441.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:53:25.00 +74:05:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-26_00-15-32_20_00sec_-9_90C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-26_00-14-41_20_00sec_-10_00C_LIGHT_0440_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-26_00-15-32_20_00sec_-9_90C_LIGHT_0441_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-26_00-14-41_20_00sec_-10_00C_LIGHT_0440_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 26.2221* 10 02 40.40 +70 44 38.2 14.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7221,14.15,0.05,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
target 20260326.2221 14.15CV 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/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_UMa-01-Q2b1x1_002048_TTUQ2b1x1_3203_h9E9B8un/fd_UMa-01-Q2b1x1_2026-03-26_00-19-13_20.00sec_-10.00C_LIGHT_0442.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_UMa-01-Q2b1x1_002048_TTUQ2b1x1_3203_h9E9B8un/fd_UMa-01-Q2b1x1_2026-03-26_00-20-02_20.00sec_-10.00C_LIGHT_0443.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:02:40.40 +70:44:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20_00sec_-15_00C_LIGHT_0264_fits__*pix.png resample_wcs_fd_UMa-01-Q2b1x1_2026-03-26_00-20-02_20_00sec_-10_00C_LIGHT_0443_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20_00sec_-15_00C_LIGHT_0264_fits__*pix.png resample_wcs_fd_UMa-01-Q2b1x1_2026-03-26_00-19-13_20_00sec_-10_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20_00sec_-15_00C_LIGHT_0264_fits__*pix.png resample_wcs_fd_UMa-01-Q2b1x1_2026-03-26_00-20-02_20_00sec_-10_00C_LIGHT_0443_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20_00sec_-15_00C_LIGHT_0264_fits__*pix.png resample_wcs_fd_UMa-01-Q2b1x1_2026-03-26_00-19-13_20_00sec_-10_00C_LIGHT_0442_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 26.2221* 09 55 41.00 +72 12 08.8 14.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7221,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2221 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_UMa-01-Q2b1x1_002048_TTUQ2b1x1_3203_h9E9B8un/fd_UMa-01-Q2b1x1_2026-03-26_00-19-13_20.00sec_-10.00C_LIGHT_0442.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_UMa-01-Q2b1x1_002048_TTUQ2b1x1_3203_h9E9B8un/fd_UMa-01-Q2b1x1_2026-03-26_00-20-02_20.00sec_-10.00C_LIGHT_0443.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:55:41.00 +72:12:08.8 ;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_UMa-01-Q2b1x1_2026-02-22_00-18-30_20_00sec_-15_00C_LIGHT_0264_fits__*pix.png resample_wcs_fd_UMa-01-Q2b1x1_2026-03-26_00-20-02_20_00sec_-10_00C_LIGHT_0443_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20_00sec_-15_00C_LIGHT_0264_fits__*pix.png resample_wcs_fd_UMa-01-Q2b1x1_2026-03-26_00-19-13_20_00sec_-10_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20_00sec_-15_00C_LIGHT_0264_fits__*pix.png resample_wcs_fd_UMa-01-Q2b1x1_2026-03-26_00-20-02_20_00sec_-10_00C_LIGHT_0443_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20_00sec_-15_00C_LIGHT_0264_fits__*pix.png resample_wcs_fd_UMa-01-Q2b1x1_2026-03-26_00-19-13_20_00sec_-10_00C_LIGHT_0442_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,2461125.7376,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2376 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-06-Q2b1x1_2026-03-19_06-42-17_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Dra-06-Q2b1x1_004303_TTUQ2b1x1_9480_VhrskM5i/fd_Dra-06-Q2b1x1_2026-03-26_00-41-33_20.00sec_-10.00C_LIGHT_0462.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Dra-06-Q2b1x1_004303_TTUQ2b1x1_9480_VhrskM5i/fd_Dra-06-Q2b1x1_2026-03-26_00-42-19_20.00sec_-10.00C_LIGHT_0463.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:08:04.54 +62:15:49.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-06-Q2b1x1_2026-03-19_06-42-17_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Dra-06-Q2b1x1_2026-03-26_00-42-19_20_00sec_-10_00C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-06-Q2b1x1_2026-03-19_06-42-17_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Dra-06-Q2b1x1_2026-03-26_00-41-33_20_00sec_-10_00C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-06-Q2b1x1_2026-03-19_06-42-17_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Dra-06-Q2b1x1_2026-03-26_00-42-19_20_00sec_-10_00C_LIGHT_0463_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-06-Q2b1x1_2026-03-19_06-42-17_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Dra-06-Q2b1x1_2026-03-26_00-41-33_20_00sec_-10_00C_LIGHT_0462_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2522 2461125.7522 13.49 12:36:15.37 +43:21:24.5
132.67852 73.48297 galactic CVn Second-epoch detections are separated by 0.8" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:36:15.37 +43:21:24.5 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7522,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2522 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CVn-01-Q2b1x1_2026-02-22_02-21-05_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-01-Q2b1x1_2026-02-22_02-21-58_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_CVn-01-Q2b1x1_010419_TTUQ2b1x1_26908_9R28EkPY/fd_CVn-01-Q2b1x1_2026-03-26_01-02-39_20.00sec_-10.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_CVn-01-Q2b1x1_010419_TTUQ2b1x1_26908_9R28EkPY/fd_CVn-01-Q2b1x1_2026-03-26_01-03-24_20.00sec_-10.00C_LIGHT_0483.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:36:15.37 +43:21:24.5 ;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_CVn-01-Q2b1x1_2026-02-22_02-21-05_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_CVn-01-Q2b1x1_2026-03-26_01-03-24_20_00sec_-10_00C_LIGHT_0483_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CVn-01-Q2b1x1_2026-02-22_02-21-05_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_CVn-01-Q2b1x1_2026-03-26_01-02-39_20_00sec_-10_00C_LIGHT_0482_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CVn-01-Q2b1x1_2026-02-22_02-21-05_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_CVn-01-Q2b1x1_2026-03-26_01-03-24_20_00sec_-10_00C_LIGHT_0483_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CVn-01-Q2b1x1_2026-02-22_02-21-05_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_CVn-01-Q2b1x1_2026-03-26_01-02-39_20_00sec_-10_00C_LIGHT_0482_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2550 2461125.7550 14.13 14:57:00.90 +48:23:14.8
82.56250 57.71742 galactic Boo Second-epoch detections are separated by 1.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J224.2554+48.3828 | 14:57:00.90 +48:23:14.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J224.2554+48.3828,2461125.7550,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J224.2554+48.3828 20260326.2550 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Boo-02-Q2b1x1_2026-03-22_05-51-31_20.00sec_-15.00C_LIGHT_0345.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-02-Q2b1x1_010821_TTUQ2b1x1_5712_SyXb8CDA/fd_Boo-02-Q2b1x1_2026-03-26_01-06-35_20.00sec_-10.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-02-Q2b1x1_010821_TTUQ2b1x1_5712_SyXb8CDA/fd_Boo-02-Q2b1x1_2026-03-26_01-07-21_20.00sec_-10.00C_LIGHT_0487.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:57:00.90 +48:23:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-02-Q2b1x1_2026-03-22_05-51-31_20_00sec_-15_00C_LIGHT_0345_fits__*pix.png resample_wcs_fd_Boo-02-Q2b1x1_2026-03-26_01-07-21_20_00sec_-10_00C_LIGHT_0487_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-02-Q2b1x1_2026-03-22_05-51-31_20_00sec_-15_00C_LIGHT_0345_fits__*pix.png resample_wcs_fd_Boo-02-Q2b1x1_2026-03-26_01-06-35_20_00sec_-10_00C_LIGHT_0486_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-02-Q2b1x1_2026-03-22_05-51-31_20_00sec_-15_00C_LIGHT_0345_fits__*pix.png resample_wcs_fd_Boo-02-Q2b1x1_2026-03-26_01-07-21_20_00sec_-10_00C_LIGHT_0487_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-02-Q2b1x1_2026-03-22_05-51-31_20_00sec_-15_00C_LIGHT_0345_fits__*pix.png resample_wcs_fd_Boo-02-Q2b1x1_2026-03-26_01-06-35_20_00sec_-10_00C_LIGHT_0486_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2618 2461125.7618 12.13 12:15:38.93 +36:19:38.4
160.25581 78.07366 galactic CVn Second-epoch detections are separated by 0.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J183.9143+36.3264 | 12:15:38.93 +36:19:38.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J183.9143+36.3264,2461125.7618,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J183.9143+36.3264 20260326.2618 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-27_02-01-33_20.00sec_-14.90C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_UMa-13-Q2b1x1_011748_TTUQ2b1x1_6711_ChvTGcay/fd_UMa-13-Q2b1x1_2026-03-26_01-16-21_20.00sec_-10.00C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_UMa-13-Q2b1x1_011748_TTUQ2b1x1_6711_ChvTGcay/fd_UMa-13-Q2b1x1_2026-03-26_01-17-09_20.00sec_-10.00C_LIGHT_0495.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:15:38.93 +36:19:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-13-Q2b1x1_2026-02-27_02-01-33_20_00sec_-14_90C_LIGHT_0082_fits__*pix.png resample_wcs_fd_UMa-13-Q2b1x1_2026-03-26_01-17-09_20_00sec_-10_00C_LIGHT_0495_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-13-Q2b1x1_2026-02-27_02-01-33_20_00sec_-14_90C_LIGHT_0082_fits__*pix.png resample_wcs_fd_UMa-13-Q2b1x1_2026-03-26_01-16-21_20_00sec_-10_00C_LIGHT_0494_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-13-Q2b1x1_2026-02-27_02-01-33_20_00sec_-14_90C_LIGHT_0082_fits__*pix.png resample_wcs_fd_UMa-13-Q2b1x1_2026-03-26_01-17-09_20_00sec_-10_00C_LIGHT_0495_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-13-Q2b1x1_2026-02-27_02-01-33_20_00sec_-14_90C_LIGHT_0082_fits__*pix.png resample_wcs_fd_UMa-13-Q2b1x1_2026-03-26_01-16-21_20_00sec_-10_00C_LIGHT_0494_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,2461125.7690,14.05,0.05,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
target 20260326.2690 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/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Hya-14-Q2b1x1_012948_TTUQ2b1x1_1724_N6qvlpQC/fd_Hya-14-Q2b1x1_2026-03-26_01-25-23_20.00sec_-10.00C_LIGHT_0504.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Hya-14-Q2b1x1_012948_TTUQ2b1x1_1724_N6qvlpQC/fd_Hya-14-Q2b1x1_2026-03-26_01-29-05_20.00sec_-10.00C_LIGHT_0505.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:19:29.06 -28:46:04.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20_00sec_-15_00C_LIGHT_0106_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-03-26_01-29-05_20_00sec_-10_00C_LIGHT_0505_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20_00sec_-15_00C_LIGHT_0106_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-03-26_01-25-23_20_00sec_-10_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20_00sec_-15_00C_LIGHT_0106_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-03-26_01-29-05_20_00sec_-10_00C_LIGHT_0505_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20_00sec_-15_00C_LIGHT_0106_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-03-26_01-25-23_20_00sec_-10_00C_LIGHT_0504_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2712 2461125.7712 13.62 17:34:43.04 +40:55:40.0
66.29394 31.30771 galactic Her Second-epoch detections are separated by 2.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1344183205823151104 | 17:34:40.49 +40:56:07.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.2712* 17 34 43.04 +40 55 40.0 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 1344183205823151104,2461125.7712,13.62,0.05,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 1344183205823151104 20260326.2712 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-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:34:43.04 +40:55:40.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20_00sec_-10_00C_LIGHT_0507_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20_00sec_-10_00C_LIGHT_0506_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20_00sec_-10_00C_LIGHT_0507_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20_00sec_-10_00C_LIGHT_0506_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2712 2461125.7712 13.86 17:50:38.63 +39:31:54.1
65.43810 28.04674 galactic Her Second-epoch detections are separated by 4.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J267.6632+39.5311 | 17:50:38.63 +39:31:54.1 (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 26.2712* 17 50 38.63 +39 31 54.1 13.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J267.6632+39.5311,2461125.7712,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J267.6632+39.5311 20260326.2712 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:50:38.63 +39:31:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20_00sec_-10_00C_LIGHT_0507_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20_00sec_-10_00C_LIGHT_0506_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20_00sec_-10_00C_LIGHT_0507_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20_00sec_-10_00C_LIGHT_0506_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 26.2782* 12 32 42.97 +21 20 56.2 14.7 U Com 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7782,14.73,0.05,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
target 20260326.2782 14.73CV 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/Com-03-Q2b1x1_2026-02-22_03-47-10_20.00sec_-15.00C_LIGHT_0385.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Com-03-Q2b1x1_014253_TTUQ2b1x1_25110_Qhqbgz83/fd_Com-03-Q2b1x1_2026-03-26_01-40-05_20.00sec_-10.00C_LIGHT_0518.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Com-03-Q2b1x1_014253_TTUQ2b1x1_25110_Qhqbgz83/fd_Com-03-Q2b1x1_2026-03-26_01-40-48_20.00sec_-10.00C_LIGHT_0519.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:32:42.97 +21:20:56.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Com-03-Q2b1x1_2026-02-22_03-47-10_20_00sec_-15_00C_LIGHT_0385_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-26_01-40-48_20_00sec_-10_00C_LIGHT_0519_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Com-03-Q2b1x1_2026-02-22_03-47-10_20_00sec_-15_00C_LIGHT_0385_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-26_01-40-05_20_00sec_-10_00C_LIGHT_0518_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-22_03-47-10_20_00sec_-15_00C_LIGHT_0385_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-26_01-40-48_20_00sec_-10_00C_LIGHT_0519_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-22_03-47-10_20_00sec_-15_00C_LIGHT_0385_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-26_01-40-05_20_00sec_-10_00C_LIGHT_0518_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2806 2461125.7806 13.86 15:10:37.01 +24:19:57.0
35.74087 58.62927 galactic Ser Second-epoch detections are separated by 1.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:10:37.01 +24:19:57.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.387+/-0.034 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.2806* 15 10 37.01 +24 19 57.0 13.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7806,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2806 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q2b1x1_2026-02-22_03-56-53_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-08-Q2b1x1_2026-02-22_03-57-38_20.00sec_-15.00C_LIGHT_0396.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-08-Q2b1x1_014649_TTUQ2b1x1_8915_RqP1GJfG/fd_Boo-08-Q2b1x1_2026-03-26_01-43-27_20.00sec_-10.00C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-08-Q2b1x1_014649_TTUQ2b1x1_8915_RqP1GJfG/fd_Boo-08-Q2b1x1_2026-03-26_01-44-16_20.00sec_-10.00C_LIGHT_0523.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:10:37.01 +24:19:57.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-08-Q2b1x1_2026-02-22_03-56-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Boo-08-Q2b1x1_2026-03-26_01-44-16_20_00sec_-10_00C_LIGHT_0523_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-08-Q2b1x1_2026-02-22_03-56-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Boo-08-Q2b1x1_2026-03-26_01-43-27_20_00sec_-10_00C_LIGHT_0522_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-08-Q2b1x1_2026-02-22_03-56-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Boo-08-Q2b1x1_2026-03-26_01-44-16_20_00sec_-10_00C_LIGHT_0523_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-08-Q2b1x1_2026-02-22_03-56-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Boo-08-Q2b1x1_2026-03-26_01-43-27_20_00sec_-10_00C_LIGHT_0522_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 26.2850* 12 55 22.39 +10 11 26.3 14.1 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7850,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2850 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:55:22.39 +10:11:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2850 2461125.7850 14.60 13:40:23.58 +12:13:21.8
342.91031 71.18817 galactic Boo Second-epoch detections are separated by 0.4" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3740258220884128384 | 13:40:25.90 +12:13:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3740258220884128384,2461125.7850,14.60,0.05,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
Gaia DR3 3740258220884128384 20260326.2850 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/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:40:23.58 +12:13:21.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_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,2461125.7862,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2862 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Boo-09-Q2b1x1_2026-02-22_04-16-49_20.00sec_-14.90C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-09-Q2b1x1_015645_TTUQ2b1x1_5676_e1bO3W4o/fd_Boo-09-Q2b1x1_2026-03-26_01-51-29_20.00sec_-10.00C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-09-Q2b1x1_015645_TTUQ2b1x1_5676_e1bO3W4o/fd_Boo-09-Q2b1x1_2026-03-26_01-52-18_20.00sec_-10.00C_LIGHT_0533.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:28:18.29 +13:46:45.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-09-Q2b1x1_2026-02-22_04-16-49_20_00sec_-14_90C_LIGHT_0417_fits__*pix.png resample_wcs_fd_Boo-09-Q2b1x1_2026-03-26_01-52-18_20_00sec_-10_00C_LIGHT_0533_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-09-Q2b1x1_2026-02-22_04-16-49_20_00sec_-14_90C_LIGHT_0417_fits__*pix.png resample_wcs_fd_Boo-09-Q2b1x1_2026-03-26_01-51-29_20_00sec_-10_00C_LIGHT_0532_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-09-Q2b1x1_2026-02-22_04-16-49_20_00sec_-14_90C_LIGHT_0417_fits__*pix.png resample_wcs_fd_Boo-09-Q2b1x1_2026-03-26_01-52-18_20_00sec_-10_00C_LIGHT_0533_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-09-Q2b1x1_2026-02-22_04-16-49_20_00sec_-14_90C_LIGHT_0417_fits__*pix.png resample_wcs_fd_Boo-09-Q2b1x1_2026-03-26_01-51-29_20_00sec_-10_00C_LIGHT_0532_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2862 2461125.7862 11.93 14:37:51.48 +14:48:30.5
11.87535 62.35823 galactic Boo Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1234001244385742720 | 14:37:51.54 +14:48:30.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.026 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1234001244385742720,2461125.7862,11.93,0.05,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 1234001244385742720 20260326.2862 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Boo-09-Q2b1x1_2026-02-22_04-16-49_20.00sec_-14.90C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-09-Q2b1x1_2026-02-22_04-17-37_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-09-Q2b1x1_015645_TTUQ2b1x1_5676_e1bO3W4o/fd_Boo-09-Q2b1x1_2026-03-26_01-51-29_20.00sec_-10.00C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-09-Q2b1x1_015645_TTUQ2b1x1_5676_e1bO3W4o/fd_Boo-09-Q2b1x1_2026-03-26_01-52-18_20.00sec_-10.00C_LIGHT_0533.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:37:51.48 +14:48:30.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-09-Q2b1x1_2026-02-22_04-16-49_20_00sec_-14_90C_LIGHT_0417_fits__*pix.png resample_wcs_fd_Boo-09-Q2b1x1_2026-03-26_01-52-18_20_00sec_-10_00C_LIGHT_0533_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-09-Q2b1x1_2026-02-22_04-16-49_20_00sec_-14_90C_LIGHT_0417_fits__*pix.png resample_wcs_fd_Boo-09-Q2b1x1_2026-03-26_01-51-29_20_00sec_-10_00C_LIGHT_0532_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-09-Q2b1x1_2026-02-22_04-16-49_20_00sec_-14_90C_LIGHT_0417_fits__*pix.png resample_wcs_fd_Boo-09-Q2b1x1_2026-03-26_01-52-18_20_00sec_-10_00C_LIGHT_0533_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-09-Q2b1x1_2026-02-22_04-16-49_20_00sec_-14_90C_LIGHT_0417_fits__*pix.png resample_wcs_fd_Boo-09-Q2b1x1_2026-03-26_01-51-29_20_00sec_-10_00C_LIGHT_0532_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2899 2461125.7899 13.62 15:30:06.31 +12:03:40.3
18.78967 49.92862 galactic Ser 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 | target | 15:30:06.31 +12:03:40.3 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.467+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.2899* 15 30 06.31 +12 03 40.3 13.6 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7899,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2899 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/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:30:06.31 +12:03:40.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20_00sec_-10_00C_LIGHT_0539_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20_00sec_-10_00C_LIGHT_0538_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20_00sec_-10_00C_LIGHT_0539_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20_00sec_-10_00C_LIGHT_0538_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 26.3028* 15 18 29.72 +02 07 18.1 13.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.8028,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3028 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-05-Q2b1x1_2026-02-22_05-29-54_20.00sec_-14.90C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20.00sec_-10.00C_LIGHT_0560.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-05-Q2b1x1_021848_TTUQ2b1x1_16065_pRLuVRUP/fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20.00sec_-10.00C_LIGHT_0561.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:18:29.72 +02:07:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20_00sec_-10_00C_LIGHT_0561_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20_00sec_-10_00C_LIGHT_0560_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-16-10_20_00sec_-10_00C_LIGHT_0561_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q2b1x1_2026-02-22_05-29-54_20_00sec_-14_90C_LIGHT_0565_fits__*pix.png resample_wcs_fd_Ser-05-Q2b1x1_2026-03-26_02-15-27_20_00sec_-10_00C_LIGHT_0560_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,2461125.7968,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2968 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-03-22_06-24-27_20.00sec_-14.90C_LIGHT_0376.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-02-Q2b1x1_022654_TTUQ2b1x1_3042_34kB45IO/fd_Lyr-02-Q2b1x1_2026-03-26_02-06-49_20.00sec_-10.00C_LIGHT_0550.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-02-Q2b1x1_022654_TTUQ2b1x1_3042_34kB45IO/fd_Lyr-02-Q2b1x1_2026-03-26_02-07-41_20.00sec_-10.00C_LIGHT_0551.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:20:10.94 +38:33:54.0 ;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_Lyr-02-Q2b1x1_2026-03-22_06-24-27_20_00sec_-14_90C_LIGHT_0376_fits__*pix.png resample_wcs_fd_Lyr-02-Q2b1x1_2026-03-26_02-07-41_20_00sec_-10_00C_LIGHT_0551_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-02-Q2b1x1_2026-03-22_06-24-27_20_00sec_-14_90C_LIGHT_0376_fits__*pix.png resample_wcs_fd_Lyr-02-Q2b1x1_2026-03-26_02-06-49_20_00sec_-10_00C_LIGHT_0550_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-02-Q2b1x1_2026-03-22_06-24-27_20_00sec_-14_90C_LIGHT_0376_fits__*pix.png resample_wcs_fd_Lyr-02-Q2b1x1_2026-03-26_02-07-41_20_00sec_-10_00C_LIGHT_0551_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-02-Q2b1x1_2026-03-22_06-24-27_20_00sec_-14_90C_LIGHT_0376_fits__*pix.png resample_wcs_fd_Lyr-02-Q2b1x1_2026-03-26_02-06-49_20_00sec_-10_00C_LIGHT_0550_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3133 2461125.8133 12.10 17:32:40.45 +01:34:23.3
25.11834 18.19689 galactic Oph Second-epoch detections are separated by 0.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4376389263071459712 | 17:32:40.42 +01:34:23.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4376389263071459712,2461125.8133,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4376389263071459712 20260326.3133 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-04-Q2b1x1_2026-02-22_06-23-10_20.00sec_-15.00C_LIGHT_0509.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-04-Q2b1x1_2026-02-22_06-24-02_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-04-Q2b1x1_023252_TTUQ2b1x1_1527_WvWWdsge/fd_Oph-04-Q2b1x1_2026-03-26_02-30-31_20.00sec_-10.00C_LIGHT_0574.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-04-Q2b1x1_023252_TTUQ2b1x1_1527_WvWWdsge/fd_Oph-04-Q2b1x1_2026-03-26_02-31-27_20.00sec_-10.00C_LIGHT_0575.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:32:40.45 +01:34:23.3 ;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_Oph-04-Q2b1x1_2026-02-22_06-23-10_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png resample_wcs_fd_Oph-04-Q2b1x1_2026-03-26_02-31-27_20_00sec_-10_00C_LIGHT_0575_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-04-Q2b1x1_2026-02-22_06-23-10_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png resample_wcs_fd_Oph-04-Q2b1x1_2026-03-26_02-30-31_20_00sec_-10_00C_LIGHT_0574_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-04-Q2b1x1_2026-02-22_06-23-10_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png resample_wcs_fd_Oph-04-Q2b1x1_2026-03-26_02-31-27_20_00sec_-10_00C_LIGHT_0575_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-04-Q2b1x1_2026-02-22_06-23-10_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png resample_wcs_fd_Oph-04-Q2b1x1_2026-03-26_02-30-31_20_00sec_-10_00C_LIGHT_0574_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,2461125.8097,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3097 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lib-05-Q2b1x1_023456_TTUQ2b1x1_2884_DPOma76S/fd_Lib-05-Q2b1x1_2026-03-26_02-25-29_20.00sec_-10.00C_LIGHT_0568.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lib-05-Q2b1x1_023456_TTUQ2b1x1_2884_DPOma76S/fd_Lib-05-Q2b1x1_2026-03-26_02-26-12_20.00sec_-9.90C_LIGHT_0569.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:24:10.91 -22:55:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20_00sec_-14_90C_LIGHT_0126_fits__*pix.png resample_wcs_fd_Lib-05-Q2b1x1_2026-03-26_02-26-12_20_00sec_-9_90C_LIGHT_0569_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20_00sec_-14_90C_LIGHT_0126_fits__*pix.png resample_wcs_fd_Lib-05-Q2b1x1_2026-03-26_02-25-29_20_00sec_-10_00C_LIGHT_0568_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20_00sec_-14_90C_LIGHT_0126_fits__*pix.png resample_wcs_fd_Lib-05-Q2b1x1_2026-03-26_02-26-12_20_00sec_-9_90C_LIGHT_0569_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20_00sec_-14_90C_LIGHT_0126_fits__*pix.png resample_wcs_fd_Lib-05-Q2b1x1_2026-03-26_02-25-29_20_00sec_-10_00C_LIGHT_0568_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3120 2461125.8120 13.16 20:27:03.87 +53:51:27.8
89.85030 8.94662 galactic Cyg Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.7636+53.8558 | 20:27:03.87 +53:51:27.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.287+/- (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
ATO J306.7636+53.8558,2461125.8120,13.16,0.05,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 J306.7636+53.8558 20260326.3120 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/Cyg-01-Q2b1x1_2026-03-22_05-41-19_20.00sec_-15.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-01-Q2b1x1_023852_TTUQ2b1x1_22903_SU4NIMf3/fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20.00sec_-10.00C_LIGHT_0572.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-01-Q2b1x1_023852_TTUQ2b1x1_22903_SU4NIMf3/fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20.00sec_-10.00C_LIGHT_0573.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:03.87 +53:51:27.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20_00sec_-10_00C_LIGHT_0573_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20_00sec_-10_00C_LIGHT_0572_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20_00sec_-10_00C_LIGHT_0573_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20_00sec_-10_00C_LIGHT_0572_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3120 2461125.8120 13.69 19:57:35.92 +51:18:24.1
85.24658 11.39099 galactic Cyg Second-epoch detections are separated by 7.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.4121+51.3062 | 19:57:35.92 +51:18:24.1 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.4121+51.3062,2461125.8120,13.69,0.05,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 J299.4121+51.3062 20260326.3120 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/Cyg-01-Q2b1x1_2026-03-22_05-41-19_20.00sec_-15.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-01-Q2b1x1_023852_TTUQ2b1x1_22903_SU4NIMf3/fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20.00sec_-10.00C_LIGHT_0572.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-01-Q2b1x1_023852_TTUQ2b1x1_22903_SU4NIMf3/fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20.00sec_-10.00C_LIGHT_0573.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:35.92 +51:18:24.1 ;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_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20_00sec_-10_00C_LIGHT_0573_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20_00sec_-10_00C_LIGHT_0572_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20_00sec_-10_00C_LIGHT_0573_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20_00sec_-10_00C_LIGHT_0572_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,2461125.8120,13.05,0.05,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 20260326.3120 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/Cyg-01-Q2b1x1_2026-03-22_05-41-19_20.00sec_-15.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-01-Q2b1x1_2026-03-22_05-42-30_20.00sec_-14.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-01-Q2b1x1_023852_TTUQ2b1x1_22903_SU4NIMf3/fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20.00sec_-10.00C_LIGHT_0572.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-01-Q2b1x1_023852_TTUQ2b1x1_22903_SU4NIMf3/fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20.00sec_-10.00C_LIGHT_0573.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:26:37.03 +54:20:36.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20_00sec_-10_00C_LIGHT_0573_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20_00sec_-10_00C_LIGHT_0572_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20_00sec_-10_00C_LIGHT_0573_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20_00sec_-10_00C_LIGHT_0572_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3120 2461125.8120 12.96 20:24:27.40 +53:06:24.6
89.00126 8.84322 galactic Cyg Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:24:27.40 +53:06:24.6 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.8120,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3120 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-01-Q2b1x1_2026-03-22_05-41-19_20.00sec_-15.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-01-Q2b1x1_2026-03-22_05-42-30_20.00sec_-14.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-01-Q2b1x1_023852_TTUQ2b1x1_22903_SU4NIMf3/fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20.00sec_-10.00C_LIGHT_0572.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-01-Q2b1x1_023852_TTUQ2b1x1_22903_SU4NIMf3/fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20.00sec_-10.00C_LIGHT_0573.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:27.40 +53:06:24.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20_00sec_-10_00C_LIGHT_0573_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20_00sec_-10_00C_LIGHT_0572_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-29-35_20_00sec_-10_00C_LIGHT_0573_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q2b1x1_2026-03-22_05-41-19_20_00sec_-15_00C_LIGHT_0335_fits__*pix.png resample_wcs_fd_Cyg-01-Q2b1x1_2026-03-26_02-28-41_20_00sec_-10_00C_LIGHT_0572_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3160 2461125.8160 13.89 15:15:04.39 -10:05:10.5
350.95614 39.03905 galactic Lib Second-epoch detections are separated by 7.6" and 11.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J228.7673-10.0861 | 15:15:04.39 -10:05:10.5 (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 J228.7673-10.0861,2461125.8160,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J228.7673-10.0861 20260326.3160 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-02-27_03-51-48_20.00sec_-14.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lib-02-Q2b1x1_024252_TTUQ2b1x1_5065_Ugjvb2AS/fd_Lib-02-Q2b1x1_2026-03-26_02-34-25_20.00sec_-10.00C_LIGHT_0578.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lib-02-Q2b1x1_024252_TTUQ2b1x1_5065_Ugjvb2AS/fd_Lib-02-Q2b1x1_2026-03-26_02-35-16_20.00sec_-10.00C_LIGHT_0579.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:15:04.39 -10:05:10.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-02-Q2b1x1_2026-02-27_03-51-48_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png resample_wcs_fd_Lib-02-Q2b1x1_2026-03-26_02-35-16_20_00sec_-10_00C_LIGHT_0579_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-02-Q2b1x1_2026-02-27_03-51-48_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png resample_wcs_fd_Lib-02-Q2b1x1_2026-03-26_02-34-25_20_00sec_-10_00C_LIGHT_0578_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-02-Q2b1x1_2026-02-27_03-51-48_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png resample_wcs_fd_Lib-02-Q2b1x1_2026-03-26_02-35-16_20_00sec_-10_00C_LIGHT_0579_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-02-Q2b1x1_2026-02-27_03-51-48_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png resample_wcs_fd_Lib-02-Q2b1x1_2026-03-26_02-34-25_20_00sec_-10_00C_LIGHT_0578_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3109 2461125.8109 13.74 19:44:03.44 +44:09:00.9
77.75453 9.92050 galactic Cyg Second-epoch detections are separated by 6.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:44:03.44 +44:09:00.9 (user input) | T | P | (position from user input) SpType: F5V 2016A&A...594A..39F KIC 8245752
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.8109,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3109 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyr-01-Q2b1x1_2026-03-22_05-59-53_20.00sec_-14.90C_LIGHT_0353.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-01-Q2b1x1_024051_TTUQ2b1x1_29807_fyYsRkg7/fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20.00sec_-10.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-01-Q2b1x1_024051_TTUQ2b1x1_29807_fyYsRkg7/fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20.00sec_-10.00C_LIGHT_0571.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:03.44 +44:09:00.9 ;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_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20_00sec_-10_00C_LIGHT_0571_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20_00sec_-10_00C_LIGHT_0570_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20_00sec_-10_00C_LIGHT_0571_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20_00sec_-10_00C_LIGHT_0570_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3109 2461125.8109 13.69 19:32:29.98 +46:02:34.2
78.51565 12.60063 galactic Cyg Second-epoch detections are separated by 2.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.1416+46.0368 | 19:32:29.98 +46:02:34.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4V 2016A&A...594A..39F KIC 9468053
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.1416+46.0368,2461125.8109,13.69,0.05,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 J293.1416+46.0368 20260326.3109 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/Lyr-01-Q2b1x1_2026-03-22_05-59-53_20.00sec_-14.90C_LIGHT_0353.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-01-Q2b1x1_024051_TTUQ2b1x1_29807_fyYsRkg7/fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20.00sec_-10.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-01-Q2b1x1_024051_TTUQ2b1x1_29807_fyYsRkg7/fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20.00sec_-10.00C_LIGHT_0571.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:29.98 +46:02:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20_00sec_-10_00C_LIGHT_0571_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20_00sec_-10_00C_LIGHT_0570_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20_00sec_-10_00C_LIGHT_0571_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20_00sec_-10_00C_LIGHT_0570_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,2461125.8109,13.64,0.05,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 20260326.3109 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/Lyr-01-Q2b1x1_2026-03-22_05-59-53_20.00sec_-14.90C_LIGHT_0353.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-01-Q2b1x1_024051_TTUQ2b1x1_29807_fyYsRkg7/fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20.00sec_-10.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-01-Q2b1x1_024051_TTUQ2b1x1_29807_fyYsRkg7/fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20.00sec_-10.00C_LIGHT_0571.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:18:50.37 +41:56:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20_00sec_-10_00C_LIGHT_0571_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20_00sec_-10_00C_LIGHT_0570_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20_00sec_-10_00C_LIGHT_0571_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20_00sec_-10_00C_LIGHT_0570_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3109 2461125.8109 14.04 19:07:17.49 +47:27:46.6
78.04370 17.12149 galactic Lyr Second-epoch detections are separated by 1.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.8229+47.4631 | 19:07:14.94 +47:27:39.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.339+/-0.075 (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 J286.8229+47.4631,2461125.8109,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.8229+47.4631 20260326.3109 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyr-01-Q2b1x1_2026-03-22_05-59-53_20.00sec_-14.90C_LIGHT_0353.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-01-Q2b1x1_024051_TTUQ2b1x1_29807_fyYsRkg7/fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20.00sec_-10.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-01-Q2b1x1_024051_TTUQ2b1x1_29807_fyYsRkg7/fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20.00sec_-10.00C_LIGHT_0571.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:07:17.49 +47:27:46.6 ;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_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20_00sec_-10_00C_LIGHT_0571_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20_00sec_-10_00C_LIGHT_0570_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-55_20_00sec_-10_00C_LIGHT_0571_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q2b1x1_2026-03-22_05-59-53_20_00sec_-14_90C_LIGHT_0353_fits__*pix.png resample_wcs_fd_Lyr-01-Q2b1x1_2026-03-26_02-27-09_20_00sec_-10_00C_LIGHT_0570_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,2461125.8187,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3187 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-05-Q2b1x1_025052_TTUQ2b1x1_16728_IZkCxGEh/fd_Cep-05-Q2b1x1_2026-03-26_02-38-15_20.00sec_-10.00C_LIGHT_0582.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-05-Q2b1x1_025052_TTUQ2b1x1_16728_IZkCxGEh/fd_Cep-05-Q2b1x1_2026-03-26_02-39-10_20.00sec_-10.00C_LIGHT_0583.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:51.29 +65:20:28.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-26_02-39-10_20_00sec_-10_00C_LIGHT_0583_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-26_02-38-15_20_00sec_-10_00C_LIGHT_0582_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-26_02-39-10_20_00sec_-10_00C_LIGHT_0583_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-26_02-38-15_20_00sec_-10_00C_LIGHT_0582_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 26.3213* 18 12 53.74 +25 05 54.6 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
target,2461125.8213,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3213 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-08-Q2b1x1_2026-02-22_05-07-51_20.00sec_-15.00C_LIGHT_0541.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-08-Q2b1x1_025251_TTUQ2b1x1_29404_OVoW9Plq/fd_Her-08-Q2b1x1_2026-03-26_02-42-05_20.00sec_-9.90C_LIGHT_0586.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-08-Q2b1x1_025251_TTUQ2b1x1_29404_OVoW9Plq/fd_Her-08-Q2b1x1_2026-03-26_02-42-52_20.00sec_-10.00C_LIGHT_0587.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:12:53.74 +25:05:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-08-Q2b1x1_2026-02-22_05-07-51_20_00sec_-15_00C_LIGHT_0541_fits__*pix.png resample_wcs_fd_Her-08-Q2b1x1_2026-03-26_02-42-52_20_00sec_-10_00C_LIGHT_0587_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-08-Q2b1x1_2026-02-22_05-07-51_20_00sec_-15_00C_LIGHT_0541_fits__*pix.png resample_wcs_fd_Her-08-Q2b1x1_2026-03-26_02-42-05_20_00sec_-9_90C_LIGHT_0586_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-08-Q2b1x1_2026-02-22_05-07-51_20_00sec_-15_00C_LIGHT_0541_fits__*pix.png resample_wcs_fd_Her-08-Q2b1x1_2026-03-26_02-42-52_20_00sec_-10_00C_LIGHT_0587_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-08-Q2b1x1_2026-02-22_05-07-51_20_00sec_-15_00C_LIGHT_0541_fits__*pix.png resample_wcs_fd_Her-08-Q2b1x1_2026-03-26_02-42-05_20_00sec_-9_90C_LIGHT_0586_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3213 2461125.8213 12.46 18:53:41.69 +20:24:50.4
51.49076 8.67526 galactic Her Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4519095186492162688 | 18:53:41.77 +20:24:49.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.179+/-0.035 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.3213* 18 53 41.69 +20 24 50.4 12.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4519095186492162688,2461125.8213,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4519095186492162688 20260326.3213 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/Her-08-Q2b1x1_2026-02-22_05-07-51_20.00sec_-15.00C_LIGHT_0541.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-08-Q2b1x1_2026-02-22_05-08-38_20.00sec_-14.90C_LIGHT_0542.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-08-Q2b1x1_025251_TTUQ2b1x1_29404_OVoW9Plq/fd_Her-08-Q2b1x1_2026-03-26_02-42-05_20.00sec_-9.90C_LIGHT_0586.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-08-Q2b1x1_025251_TTUQ2b1x1_29404_OVoW9Plq/fd_Her-08-Q2b1x1_2026-03-26_02-42-52_20.00sec_-10.00C_LIGHT_0587.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:53:41.69 +20:24:50.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-08-Q2b1x1_2026-02-22_05-07-51_20_00sec_-15_00C_LIGHT_0541_fits__*pix.png resample_wcs_fd_Her-08-Q2b1x1_2026-03-26_02-42-52_20_00sec_-10_00C_LIGHT_0587_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-08-Q2b1x1_2026-02-22_05-07-51_20_00sec_-15_00C_LIGHT_0541_fits__*pix.png resample_wcs_fd_Her-08-Q2b1x1_2026-03-26_02-42-05_20_00sec_-9_90C_LIGHT_0586_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-08-Q2b1x1_2026-02-22_05-07-51_20_00sec_-15_00C_LIGHT_0541_fits__*pix.png resample_wcs_fd_Her-08-Q2b1x1_2026-03-26_02-42-52_20_00sec_-10_00C_LIGHT_0587_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-08-Q2b1x1_2026-02-22_05-07-51_20_00sec_-15_00C_LIGHT_0541_fits__*pix.png resample_wcs_fd_Her-08-Q2b1x1_2026-03-26_02-42-05_20_00sec_-9_90C_LIGHT_0586_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3334 2461125.8334 13.09 17:39:28.30 +03:24:53.5
27.66148 17.55190 galactic Oph Second-epoch detections are separated by 1.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:39:28.30 +03:24:53.5 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.8334,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3334 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-03-Q2b1x1_2026-02-22_05-28-08_20.00sec_-14.90C_LIGHT_0563.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-03-Q2b1x1_030103_TTUQ2b1x1_7122_eldVBzXf/fd_Oph-03-Q2b1x1_2026-03-26_02-59-27_20.00sec_-10.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-03-Q2b1x1_030103_TTUQ2b1x1_7122_eldVBzXf/fd_Oph-03-Q2b1x1_2026-03-26_03-00-17_20.00sec_-10.00C_LIGHT_0597.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:39:28.30 +03:24:53.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-26_03-00-17_20_00sec_-10_00C_LIGHT_0597_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-26_02-59-27_20_00sec_-10_00C_LIGHT_0596_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-26_03-00-17_20_00sec_-10_00C_LIGHT_0597_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-03-Q2b1x1_2026-02-22_05-28-08_20_00sec_-14_90C_LIGHT_0563_fits__*pix.png resample_wcs_fd_Oph-03-Q2b1x1_2026-03-26_02-59-27_20_00sec_-10_00C_LIGHT_0596_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3322 2461125.8322 13.31 19:28:12.35 +30:33:48.0
64.15589 6.28338 galactic Cyg Second-epoch detections are separated by 1.8" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.0508+30.5635 | 19:28:12.35 +30:33:48.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.359+/-0.038 (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 J292.0508+30.5635,2461125.8322,13.31,0.05,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 J292.0508+30.5635 20260326.3322 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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-03-Q2b1x1_025918_TTUQ2b1x1_13452_PZ0KGimg/fd_Lyr-03-Q2b1x1_2026-03-26_02-57-53_20.00sec_-10.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lyr-03-Q2b1x1_025918_TTUQ2b1x1_13452_PZ0KGimg/fd_Lyr-03-Q2b1x1_2026-03-26_02-58-37_20.00sec_-10.00C_LIGHT_0595.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:12.35 +30:33:48.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-26_02-58-37_20_00sec_-10_00C_LIGHT_0595_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-26_02-57-53_20_00sec_-10_00C_LIGHT_0594_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-26_02-58-37_20_00sec_-10_00C_LIGHT_0595_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-26_02-57-53_20_00sec_-10_00C_LIGHT_0594_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3416 2461125.8416 13.57 20:02:00.22 +36:12:13.9
72.57787 2.96292 galactic Cyg Second-epoch detections are separated by 8.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.5021+36.2086 | 20:02:00.22 +36:12:13.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.5021+36.2086,2461125.8416,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.5021+36.2086 20260326.3416 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20.00sec_-14.90C_LIGHT_0600.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20.00sec_-15.00C_LIGHT_0601.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:02:00.22 +36:12:13.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3416 2461125.8416 13.10 19:45:54.89 +33:43:28.1
68.75223 4.52328 galactic Cyg Second-epoch detections are separated by 8.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.4756+33.7234 | 19:45:54.89 +33:43:28.1 (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 J296.4756+33.7234,2461125.8416,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.4756+33.7234 20260326.3416 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20.00sec_-14.90C_LIGHT_0600.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20.00sec_-15.00C_LIGHT_0601.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:54.89 +33:43:28.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3416 2461125.8416 13.45 19:39:36.70 +37:05:29.3
71.07489 7.28887 galactic Cyg Second-epoch detections are separated by 0.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.8957+37.0901 | 19:39:36.70 +37:05:29.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.8957+37.0901,2461125.8416,13.45,0.05,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 J294.8957+37.0901 20260326.3416 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-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20.00sec_-14.90C_LIGHT_0600.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20.00sec_-15.00C_LIGHT_0601.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:36.70 +37:05:29.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3416 2461125.8416 13.48 19:36:36.60 +36:38:07.1
70.38180 7.59909 galactic Cyg Second-epoch detections are separated by 8.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.1546+36.6363 | 19:36:36.60 +36:38:07.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.325+/-0.050 (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 J294.1546+36.6363,2461125.8416,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.1546+36.6363 20260326.3416 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20.00sec_-14.90C_LIGHT_0600.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20.00sec_-15.00C_LIGHT_0601.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:36:36.60 +36:38:07.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3416 2461125.8416 13.60 19:45:43.67 +40:05:51.4
74.31154 7.69674 galactic Cyg Second-epoch detections are separated by 5.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.4422+40.0933 | 19:45:43.67 +40:05:51.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.4422+40.0933,2461125.8416,13.60,0.05,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
ATO J296.4422+40.0933 20260326.3416 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20.00sec_-14.90C_LIGHT_0600.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20.00sec_-15.00C_LIGHT_0601.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:43.67 +40:05:51.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_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,2461125.8416,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3416 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20.00sec_-14.90C_LIGHT_0600.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20.00sec_-15.00C_LIGHT_0601.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:35:03.65 +34:12:52.7 ;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_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3416 2461125.8416 13.63 19:41:51.35 +39:09:59.6
73.12497 7.89818 galactic Cyg Second-epoch detections are separated by 3.9" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.4650+39.1649 | 19:41:48.57 +39:10:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.4650+39.1649,2461125.8416,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.4650+39.1649 20260326.3416 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20.00sec_-14.90C_LIGHT_0600.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20.00sec_-15.00C_LIGHT_0601.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:51.35 +39:09:59.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3416 2461125.8416 12.73 20:08:59.72 +37:43:39.3
74.61465 2.59808 galactic Cyg Second-epoch detections are separated by 0.4" 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 J302.2604+37.7195 | 20:08:59.74 +37:43:40.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.804+/-0.024 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.2604+37.7195,2461125.8416,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J302.2604+37.7195 20260326.3416 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20.00sec_-14.90C_LIGHT_0600.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-05-Q2b1x1_031248_TTUQ2b1x1_5229_nzTwPLzU/fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20.00sec_-15.00C_LIGHT_0601.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:08:59.72 +37:43:39.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-12-08_20_00sec_-15_00C_LIGHT_0601_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-02-27_05-44-43_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-03-26_03-11-21_20_00sec_-14_90C_LIGHT_0600_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3427 2461125.8427 13.88 18:32:04.11 +12:18:20.5
41.81019 9.82180 galactic Her Second-epoch detections are separated by 3.9" 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 | NSVS J1832025+121836 | 18:32:01.67 +12:18:26.6 (Gaia DR3) | SRB (local) | (local) | Gaia3var=VARIABLE SpType: M6 (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 26.3427* 18 32 04.11 +12 18 20.5 13.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1832025+121836,2461125.8427,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1832025+121836 20260326.3427 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_031433_TTUQ2b1x1_24389_6k0T6Kyx/fd_Her-10-Q2b1x1_2026-03-26_03-12-58_20.00sec_-14.90C_LIGHT_0602.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_031433_TTUQ2b1x1_24389_6k0T6Kyx/fd_Her-10-Q2b1x1_2026-03-26_03-13-42_20.00sec_-15.00C_LIGHT_0603.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:32:04.11 +12:18:20.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_03-13-42_20_00sec_-15_00C_LIGHT_0603_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_2026-03-26_03-12-58_20_00sec_-14_90C_LIGHT_0602_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_2026-03-26_03-13-42_20_00sec_-15_00C_LIGHT_0603_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_2026-03-26_03-12-58_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3427 2461125.8427 13.90 18:42:59.82 +13:03:55.4
43.68317 7.75885 galactic Her Second-epoch detections are separated by 4.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4505610707168326272 | 18:42:59.79 +13:04:39.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.524+/-0.164 (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 26.3427* 18 42 59.82 +13 03 55.4 13.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4505610707168326272,2461125.8427,13.90,0.05,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 4505610707168326272 20260326.3427 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_031433_TTUQ2b1x1_24389_6k0T6Kyx/fd_Her-10-Q2b1x1_2026-03-26_03-12-58_20.00sec_-14.90C_LIGHT_0602.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_031433_TTUQ2b1x1_24389_6k0T6Kyx/fd_Her-10-Q2b1x1_2026-03-26_03-13-42_20.00sec_-15.00C_LIGHT_0603.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:42:59.82 +13:03:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_03-13-42_20_00sec_-15_00C_LIGHT_0603_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_2026-03-26_03-12-58_20_00sec_-14_90C_LIGHT_0602_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_2026-03-26_03-13-42_20_00sec_-15_00C_LIGHT_0603_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_2026-03-26_03-12-58_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3427 2461125.8427 12.34 19:03:19.80 +13:24:15.8
46.21427 3.48601 galactic Aql Second-epoch detections are separated by 1.2" 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 4314267367200009984 | 19:03:19.90 +13:24:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.840+/-0.025 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4314267367200009984,2461125.8427,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4314267367200009984 20260326.3427 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-55-08_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_031433_TTUQ2b1x1_24389_6k0T6Kyx/fd_Her-10-Q2b1x1_2026-03-26_03-12-58_20.00sec_-14.90C_LIGHT_0602.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_031433_TTUQ2b1x1_24389_6k0T6Kyx/fd_Her-10-Q2b1x1_2026-03-26_03-13-42_20.00sec_-15.00C_LIGHT_0603.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:03:19.80 +13:24:15.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_03-13-42_20_00sec_-15_00C_LIGHT_0603_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_2026-03-26_03-12-58_20_00sec_-14_90C_LIGHT_0602_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_2026-03-26_03-13-42_20_00sec_-15_00C_LIGHT_0603_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_2026-03-26_03-12-58_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3468 2461125.8468 12.44 16:23:42.27 -26:29:30.8
351.01738 15.97552 galactic Sco Second-epoch detections are separated by 2.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6045466365218154240 | 16:23:44.05 -26:30:06.5 (Gaia DR3) | S (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
Gaia DR3 6045466365218154240,2461125.8468,12.44,0.05,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 6045466365218154240 20260326.3468 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-02-Q2b1x1_032018_TTUQ2b1x1_26348_oHwMY8SL/fd_Sco-02-Q2b1x1_2026-03-26_03-18-53_20.00sec_-14.90C_LIGHT_0606.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-02-Q2b1x1_032018_TTUQ2b1x1_26348_oHwMY8SL/fd_Sco-02-Q2b1x1_2026-03-26_03-19-41_20.00sec_-15.00C_LIGHT_0607.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:23:42.27 -26:29:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-26_03-19-41_20_00sec_-15_00C_LIGHT_0607_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-26_03-18-53_20_00sec_-14_90C_LIGHT_0606_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-26_03-19-41_20_00sec_-15_00C_LIGHT_0607_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-26_03-18-53_20_00sec_-14_90C_LIGHT_0606_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3588 2461125.8588 13.65 19:02:12.73 +25:03:42.2
56.58960 8.93220 galactic Vul Second-epoch detections are separated by 6.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J285.5429+25.0612 | 19:02:12.73 +25:03:42.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J285.5429+25.0612,2461125.8588,13.65,0.05,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
ATO J285.5429+25.0612 20260326.3588 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/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20.00sec_-14.90C_LIGHT_0610.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20.00sec_-15.00C_LIGHT_0611.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:02:12.73 +25:03:42.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3588 2461125.8588 13.03 19:32:11.92 +25:04:45.0
59.73233 2.90436 galactic Vul Second-epoch detections are separated by 3.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.0575+25.0926 | 19:32:12.49 +25:05:03.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.795+/-0.158 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.0575+25.0926,2461125.8588,13.03,0.05,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
ATO J293.0575+25.0926 20260326.3588 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20.00sec_-14.90C_LIGHT_0610.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20.00sec_-15.00C_LIGHT_0611.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:11.92 +25:04:45.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3588 2461125.8588 12.79 19:49:47.15 +25:35:14.0
62.13822 -0.29958 galactic Vul Second-epoch detections are separated by 0.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.4398+25.5859 | 19:49:47.49 +25:35:17.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.4398+25.5859,2461125.8588,12.79,0.05,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
ATO J297.4398+25.5859 20260326.3588 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/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20.00sec_-14.90C_LIGHT_0610.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20.00sec_-15.00C_LIGHT_0611.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:47.15 +25:35:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3588 2461125.8588 12.29 19:47:17.29 +21:50:01.2
58.61045 -1.70496 galactic Vul Second-epoch detections are separated by 1.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.8265+21.8342 | 19:47:17.09 +21:50:00.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.8265+21.8342,2461125.8588,12.29,0.05,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 J296.8265+21.8342 20260326.3588 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20.00sec_-14.90C_LIGHT_0610.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20.00sec_-15.00C_LIGHT_0611.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:47:17.29 +21:50:01.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3588 2461125.8588 12.68 19:49:20.98 +21:31:39.8
58.58808 -2.27282 galactic Vul Second-epoch detections are separated by 1.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1827481135313692032 | 19:49:23.10 +21:31:30.1 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.261+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1827481135313692032,2461125.8588,12.68,0.05,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 1827481135313692032 20260326.3588 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/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20.00sec_-14.90C_LIGHT_0610.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_033733_TTUQ2b1x1_2741_RRpnDS18/fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20.00sec_-15.00C_LIGHT_0611.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:20.98 +21:31:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-53_20_00sec_-15_00C_LIGHT_0611_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_03-36-07_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3738 2461125.8738 13.54 19:35:59.48 +30:46:46.7
65.14553 4.91251 galactic Cyg Second-epoch detections are separated by 4.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.9998+30.7770 | 19:35:59.00 +30:47:13.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1950ApJ...112...90M LF 2 +30 206
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.9998+30.7770,2461125.8738,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.9998+30.7770 20260326.3738 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20.00sec_-14.90C_LIGHT_0618.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20.00sec_-14.90C_LIGHT_0619.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:35:59.48 +30:46:46.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3738 2461125.8738 13.85 19:38:00.95 +28:14:33.0
63.13442 3.29775 galactic Cyg Second-epoch detections are separated by 3.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.4997+28.2450 | 19:37:59.94 +28:14:42.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.544+/-0.171 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.4997+28.2450,2461125.8738,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.4997+28.2450 20260326.3738 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20.00sec_-14.90C_LIGHT_0618.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20.00sec_-14.90C_LIGHT_0619.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:38:00.95 +28:14:33.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_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,2461125.8738,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3738 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20.00sec_-14.90C_LIGHT_0618.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20.00sec_-14.90C_LIGHT_0619.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:05.39 +33:24:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3738 2461125.8738 13.34 19:37:10.20 +31:55:53.1
66.28046 5.24709 galactic Cyg Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.2893+31.9305 | 19:37:10.20 +31:55:53.1 (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 J294.2893+31.9305,2461125.8738,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.2893+31.9305 20260326.3738 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20.00sec_-14.90C_LIGHT_0618.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20.00sec_-14.90C_LIGHT_0619.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:37:10.20 +31:55:53.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3738 2461125.8738 13.21 19:33:09.18 +33:49:30.7
67.54940 6.89191 galactic Cyg Second-epoch detections are separated by 1.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.2881+33.8175 | 19:33:08.81 +33:48:51.5 (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 J293.2881+33.8175,2461125.8738,13.21,0.05,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
ATO J293.2881+33.8175 20260326.3738 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20.00sec_-14.90C_LIGHT_0618.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20.00sec_-14.90C_LIGHT_0619.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:09.18 +33:49:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_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,2461125.8738,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3738 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20.00sec_-14.90C_LIGHT_0618.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20.00sec_-14.90C_LIGHT_0619.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:15.72 +29:54:53.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3738 2461125.8738 12.99 19:44:18.68 +30:32:28.4
65.81463 3.23541 galactic Cyg Second-epoch detections are separated by 5.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2032103994528695936 | 19:44:17.28 +30:32:59.9 (Gaia DR3) | E (local) | G (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
Gaia DR3 2032103994528695936,2461125.8738,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2032103994528695936 20260326.3738 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20.00sec_-14.90C_LIGHT_0618.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20.00sec_-14.90C_LIGHT_0619.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:18.68 +30:32:28.4 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3738 2461125.8738 13.04 19:32:01.97 +27:55:24.8
62.21623 4.29965 galactic Cyg Second-epoch detections are separated by 3.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.9994+27.9131 | 19:32:01.97 +27:55:24.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.9994+27.9131,2461125.8738,13.04,0.05,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
ATO J292.9994+27.9131 20260326.3738 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20.00sec_-14.90C_LIGHT_0618.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_035918_TTUQ2b1x1_2850_KtYsKsyQ/fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20.00sec_-14.90C_LIGHT_0619.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:01.97 +27:55:24.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-58-30_20_00sec_-14_90C_LIGHT_0619_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_03-57-45_20_00sec_-14_90C_LIGHT_0618_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 12.39 17:37:04.74 -16:36:20.0
9.50071 8.13897 galactic Oph Second-epoch detections are separated by 0.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J264.2569-16.6063 | 17:37:04.50 -16:36:10.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1V 1988MSS...C04....0H HD 159761
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J264.2569-16.6063,2461125.8765,12.39,0.05,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 J264.2569-16.6063 20260326.3765 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:37:04.74 -16:36:20.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 10.79 18:11:57.55 -19:10:07.3
11.45911 -0.32255 galactic Sgr Second-epoch detections are separated by 0.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.9850-19.1598 | 18:11:57.64 -19:10:06.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.002+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.9850-19.1598,2461125.8765,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.9850-19.1598 20260326.3765 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:57.55 -19:10:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 11.49 18:10:18.87 -18:03:47.0
12.24022 0.55160 galactic Sgr Second-epoch detections are separated by 0.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4095806986733133952 | 18:10:18.92 -18:03:47.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.648+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095806986733133952,2461125.8765,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095806986733133952 20260326.3765 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:18.87 -18:03:47.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 11.60 18:09:09.64 -19:20:42.2
10.98592 0.17084 galactic Sgr Second-epoch detections are separated by 0.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4095100133887494272 | 18:09:09.74 -19:20:42.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.830+/-0.039 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095100133887494272,2461125.8765,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095100133887494272 20260326.3765 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:09:09.64 -19:20:42.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 12.66 17:34:00.84 -17:45:25.4
8.12241 8.15518 galactic Oph Second-epoch detections are separated by 5.7" 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 | ASASSN-V J173402.66-174452.2 | 17:34:02.66 -17:44:52.3 (Gaia DR3) | SRS (local) | 14.908000000000 (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173402.66-174452.2,2461125.8765,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173402.66-174452.2 20260326.3765 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:34:00.84 -17:45:25.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 12.21 18:11:26.30 -19:16:51.0
11.30164 -0.26872 galactic Sgr Second-epoch detections are separated by 0.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4095464725072823936 | 18:11:26.35 -19:16:52.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.425+/-0.041 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095464725072823936,2461125.8765,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095464725072823936 20260326.3765 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:26.30 -19:16:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 10.81 18:09:52.85 -15:12:11.8
14.69534 2.02294 galactic Ser Second-epoch detections are separated by 0.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.4729-15.2150 | 18:09:52.91 -15:12:11.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.814+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.3765* 18 09 52.85 -15 12 11.8 10.8 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.4729-15.2150,2461125.8765,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.4729-15.2150 20260326.3765 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:09:52.85 -15:12:11.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 11.29 18:10:33.81 -19:21:17.9
11.13720 -0.12362 galactic Sgr Second-epoch detections are separated by 0.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4095091135946030592 | 18:10:33.89 -19:21:18.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.688+/-0.026 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095091135946030592,2461125.8765,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095091135946030592 20260326.3765 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:33.81 -19:21:17.9 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 12.06 18:11:41.20 -19:14:59.4
11.35702 -0.30518 galactic Sgr Second-epoch detections are separated by 0.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.9127-19.2491 | 18:11:41.26 -19:15:03.5 (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 J272.9127-19.2491,2461125.8765,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.9127-19.2491 20260326.3765 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:41.20 -19:14:59.4 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 12.07 18:10:52.03 -14:53:57.3
15.07671 1.96077 galactic Ser Second-epoch detections are separated by 0.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.7089-14.9001 | 18:10:52.12 -14:53:57.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.724+/-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 26.3765* 18 10 52.03 -14 53 57.3 12.1 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.7089-14.9001,2461125.8765,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.7089-14.9001 20260326.3765 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:52.03 -14:53:57.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 12.26 18:11:47.67 -15:48:15.8
14.39035 1.32946 galactic Ser Second-epoch detections are separated by 0.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4145793358003964288 | 18:11:47.78 -15:48:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.488+/-0.050 (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 26.3765* 18 11 47.67 -15 48 15.8 12.3 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4145793358003964288,2461125.8765,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4145793358003964288 20260326.3765 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:47.67 -15:48:15.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3765 2461125.8765 12.82 18:11:35.41 -19:36:34.2
11.03078 -0.45830 galactic Sgr Second-epoch detections are separated by 2.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4094330097791337088 | 18:11:37.65 -19:36:41.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.440+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4094330097791337088,2461125.8765,12.82,0.05,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
Gaia DR3 4094330097791337088 20260326.3765 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20.00sec_-15.00C_LIGHT_0622.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-01-Q2b1x1_040303_TTUQ2b1x1_3219_iIupxsm5/fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20.00sec_-15.00C_LIGHT_0623.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:35.41 -19:36:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-02-24_20_00sec_-15_00C_LIGHT_0623_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-26_04-01-37_20_00sec_-15_00C_LIGHT_0622_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3806 2461125.8806 13.93 19:07:46.07 +02:05:26.1
36.65751 -2.67578 galactic Aql Second-epoch detections are separated by 4.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.9376+02.0857 | 19:07:46.07 +02:05:26.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J286.9376+02.0857,2461125.8806,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.9376+02.0857 20260326.3806 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_040903_TTUQ2b1x1_28000_a0ZbPscG/fd_Aql-03-Q2b1x1_2026-03-26_04-07-33_20.00sec_-14.90C_LIGHT_0626.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_040903_TTUQ2b1x1_28000_a0ZbPscG/fd_Aql-03-Q2b1x1_2026-03-26_04-08-20_20.00sec_-15.00C_LIGHT_0627.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:07:46.07 +02:05:26.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-08-20_20_00sec_-15_00C_LIGHT_0627_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-07-33_20_00sec_-14_90C_LIGHT_0626_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-08-20_20_00sec_-15_00C_LIGHT_0627_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-07-33_20_00sec_-14_90C_LIGHT_0626_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3806 2461125.8806 14.23 18:50:12.11 -01:05:20.1
31.82189 -0.22152 galactic Aql Second-epoch detections are separated by 5.3" 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 | ASAS J185012-0104.7 | 18:50:11.51 -01:04:40.6 (Gaia DR3) | SR (local) | 2452438.00000 (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
ASAS J185012-0104.7,2461125.8806,14.23,0.05,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
ASAS J185012-0104.7 20260326.3806 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_040903_TTUQ2b1x1_28000_a0ZbPscG/fd_Aql-03-Q2b1x1_2026-03-26_04-07-33_20.00sec_-14.90C_LIGHT_0626.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_040903_TTUQ2b1x1_28000_a0ZbPscG/fd_Aql-03-Q2b1x1_2026-03-26_04-08-20_20.00sec_-15.00C_LIGHT_0627.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:50:12.11 -01:05:20.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-08-20_20_00sec_-15_00C_LIGHT_0627_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-07-33_20_00sec_-14_90C_LIGHT_0626_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-08-20_20_00sec_-15_00C_LIGHT_0627_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-07-33_20_00sec_-14_90C_LIGHT_0626_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3806 2461125.8806 13.03 18:24:51.12 -00:32:35.0
29.40542 5.66336 galactic Ser Second-epoch detections are separated by 2.2" 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 J276.2115-00.5415 | 18:24:51.12 -00:32:35.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.3806* 18 24 51.12 +00 32 35.0 13.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J276.2115-00.5415,2461125.8806,13.03,0.05,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
ATO J276.2115-00.5415 20260326.3806 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_040903_TTUQ2b1x1_28000_a0ZbPscG/fd_Aql-03-Q2b1x1_2026-03-26_04-07-33_20.00sec_-14.90C_LIGHT_0626.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_040903_TTUQ2b1x1_28000_a0ZbPscG/fd_Aql-03-Q2b1x1_2026-03-26_04-08-20_20.00sec_-15.00C_LIGHT_0627.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:24:51.12 -00:32:35.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-08-20_20_00sec_-15_00C_LIGHT_0627_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-07-33_20_00sec_-14_90C_LIGHT_0626_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-08-20_20_00sec_-15_00C_LIGHT_0627_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_04-07-33_20_00sec_-14_90C_LIGHT_0626_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3795 2461125.8795 13.67 19:06:47.02 +16:16:10.1
49.15148 4.04748 galactic Aql Second-epoch detections are separated by 3.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J286.6918+16.2707 | 19:06:47.02 +16:16:10.1 (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 J286.6918+16.2707,2461125.8795,13.67,0.05,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 J286.6918+16.2707 20260326.3795 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20.00sec_-14.90C_LIGHT_0624.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20.00sec_-14.90C_LIGHT_0625.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:06:47.02 +16:16:10.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3795 2461125.8795 13.69 19:56:06.09 +12:18:52.4
51.42522 -8.32785 galactic Aql Second-epoch detections are separated by 4.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.0182+12.3220 | 19:56:06.09 +12:18:52.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.0182+12.3220,2461125.8795,13.69,0.05,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 J299.0182+12.3220 20260326.3795 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/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20.00sec_-14.90C_LIGHT_0624.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20.00sec_-14.90C_LIGHT_0625.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:56:06.09 +12:18:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_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,2461125.8795,13.52,0.05,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 20260326.3795 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/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20.00sec_-14.90C_LIGHT_0624.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20.00sec_-14.90C_LIGHT_0625.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:06:59.99 +14:01:10.3 ;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_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3795 2461125.8795 13.55 19:41:58.58 +17:41:16.3
54.39075 -2.68956 galactic Sge Second-epoch detections are separated by 3.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.4925+17.6921 | 19:41:58.58 +17:41:16.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.4925+17.6921,2461125.8795,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.4925+17.6921 20260326.3795 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20.00sec_-14.90C_LIGHT_0624.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20.00sec_-14.90C_LIGHT_0625.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:58.58 +17:41:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3795 2461125.8795 14.40 19:38:09.79 +15:38:30.8
52.15739 -2.89906 galactic Aql Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.5445+15.6355 | 19:38:09.79 +15:38:30.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.578+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.5445+15.6355,2461125.8795,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.5445+15.6355 20260326.3795 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20.00sec_-14.90C_LIGHT_0624.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20.00sec_-14.90C_LIGHT_0625.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:38:09.79 +15:38:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3795 2461125.8795 12.92 19:29:53.70 +14:00:09.1
49.75424 -1.94223 galactic Aql Second-epoch detections are separated by 0.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.4742+14.0046 | 19:29:53.82 +14:00:16.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.4742+14.0046,2461125.8795,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.4742+14.0046 20260326.3795 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20.00sec_-14.90C_LIGHT_0624.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_040733_TTUQ2b1x1_9705_sz9nibgO/fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20.00sec_-14.90C_LIGHT_0625.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:53.70 +14:00:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-06-44_20_00sec_-14_90C_LIGHT_0625_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_04-05-57_20_00sec_-14_90C_LIGHT_0624_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3865 2461125.8865 11.97 16:53:25.34 -22:10:38.6
358.91780 13.51826 galactic Oph Second-epoch detections are separated by 0.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J253.3475-22.1702 | 16:53:25.34 -22:10:38.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9: CN2 1985PASP...97..465H NGC 6235
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J253.3475-22.1702,2461125.8865,11.97,0.05,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
ATO J253.3475-22.1702 20260326.3865 11.97CV 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/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20.00sec_-14.90C_LIGHT_0628.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-08-Q2b1x1_041733_TTUQ2b1x1_31577_fo6kNuO4/fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20.00sec_-15.00C_LIGHT_0629.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:53:25.34 -22:10:38.6 ;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_Oph-08-Q2b1x1_2026-02-27_06-14-28_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-16-44_20_00sec_-15_00C_LIGHT_0629_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Oph-08-Q2b1x1_2026-03-26_04-15-57_20_00sec_-14_90C_LIGHT_0628_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3877 2461125.8877 14.03 20:34:06.83 +41:07:52.4
80.17389 0.54811 galactic Cyg Second-epoch detections are separated by 5.4" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J308.5250+41.1358 | 20:34:06.01 +41:08:09.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B1V 2007ApJ...664.1102K [MT91] 712
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J308.5250+41.1358,2461125.8877,14.03,0.05,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
ATO J308.5250+41.1358 20260326.3877 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-17-41_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20.00sec_-15.00C_LIGHT_0631.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:34:06.83 +41:07:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_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_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3877 2461125.8877 13.57 20:56:48.32 +40:11:42.0
82.12280 -3.40053 galactic Cyg Second-epoch detections are separated by 4.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.2020+40.1816 | 20:56:50.80 +40:11:09.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.2020+40.1816,2461125.8877,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.2020+40.1816 20260326.3877 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-17-41_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20.00sec_-15.00C_LIGHT_0631.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:56:48.32 +40:11:42.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_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_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3877 2461125.8877 13.79 21:08:52.93 +41:16:06.2
84.44729 -4.40424 galactic Cyg Second-epoch detections are separated by 1.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1969343664591506560 | 21:08:52.87 +41:15:21.3 (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 1969343664591506560,2461125.8877,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1969343664591506560 20260326.3877 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-17-41_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20.00sec_-15.00C_LIGHT_0631.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:08:52.93 +41:16:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_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_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3877 2461125.8877 13.90 20:50:36.27 +39:00:21.6
80.44180 -3.24575 galactic Cyg Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.6418+39.0102 | 20:50:36.78 +39:00:48.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.624+/- (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.6418+39.0102,2461125.8877,13.90,0.05,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
ATO J312.6418+39.0102 20260326.3877 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-17-41_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20.00sec_-15.00C_LIGHT_0631.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:50:36.27 +39:00:21.6 ;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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_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_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3877 2461125.8877 14.22 21:06:10.63 +41:48:26.2
84.50517 -3.66716 galactic Cyg Second-epoch detections are separated by 2.2" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.5427+41.8088 | 21:06:10.63 +41:48:26.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J316.5427+41.8088,2461125.8877,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.5427+41.8088 20260326.3877 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-17-41_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_041918_TTUQ2b1x1_8934_b432mvWn/fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20.00sec_-15.00C_LIGHT_0631.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:06:10.63 +41:48:26.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_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_2026-03-26_04-18-28_20_00sec_-15_00C_LIGHT_0631_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_2026-03-26_04-17-41_20_00sec_-14_90C_LIGHT_0630_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,2461125.8897,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3897 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-26_19-31-09_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20.00sec_-15.00C_LIGHT_0632.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20.00sec_-15.00C_LIGHT_0633.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:23:41.19 +65:51:21.6 ;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_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3897 2461125.8897 13.99 22:01:37.60 +62:46:07.5
104.83795 6.02532 galactic Cep Second-epoch detections are separated by 1.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2204421788924944512 | 22:01:33.14 +62:46:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2204421788924944512,2461125.8897,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2204421788924944512 20260326.3897 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-26_19-31-09_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20.00sec_-15.00C_LIGHT_0632.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20.00sec_-15.00C_LIGHT_0633.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:37.60 +62:46:07.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3897 2461125.8897 13.87 22:31:54.15 +59:56:25.6
106.27787 1.65980 galactic Cep Second-epoch detections are separated by 2.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2200870851708780032 | 22:31:52.57 +59:55:49.9 (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 2200870851708780032,2461125.8897,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2200870851708780032 20260326.3897 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-26_19-31-09_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20.00sec_-15.00C_LIGHT_0632.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20.00sec_-15.00C_LIGHT_0633.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:31:54.15 +59:56:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_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,2461125.8897,14.18,0.05,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 20260326.3897 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-26_19-31-09_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20.00sec_-15.00C_LIGHT_0632.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20.00sec_-15.00C_LIGHT_0633.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:18:16.22 +64:10:27.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3897 2461125.8897 14.21 22:38:24.02 +58:08:55.8
106.10875 -0.30969 galactic Cep Second-epoch detections are separated by 3.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J339.6003+58.1505 | 22:38:24.02 +58:08:55.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J339.6003+58.1505,2461125.8897,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J339.6003+58.1505 20260326.3897 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-26_19-31-09_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20.00sec_-15.00C_LIGHT_0632.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20.00sec_-15.00C_LIGHT_0633.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:38:24.02 +58:08:55.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_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,2461125.8897,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3897 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-26_19-31-09_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20.00sec_-15.00C_LIGHT_0632.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20.00sec_-15.00C_LIGHT_0633.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:22.10 +63:17:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3897 2461125.8897 13.22 22:47:24.45 +58:18:56.0
107.23193 -0.72404 galactic Cep Second-epoch detections are separated by 1.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J224726.67+581831.7 | 22:47:26.65 +58:18:31.6 (Gaia DR3) | SR (local) | 191.996785800000 (local) | Gaia3var=VARIABLE SpType: C 1954ApJ...120..129N Case 259
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J224726.67+581831.7,2461125.8897,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J224726.67+581831.7 20260326.3897 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-26_19-31-58_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20.00sec_-15.00C_LIGHT_0632.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_042203_TTUQ2b1x1_9476_JVDeJrqc/fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20.00sec_-15.00C_LIGHT_0633.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:47:24.45 +58:18:56.0 ;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_Cep-06-Q2b1x1_2025-12-26_19-31-58_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-58_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-58_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-21-25_20_00sec_-15_00C_LIGHT_0633_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-58_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_04-20-37_20_00sec_-15_00C_LIGHT_0632_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3971 2461125.8971 14.15 20:43:47.14 +24:12:29.7
67.80384 -11.25582 galactic Vul Second-epoch detections are separated by 8.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J310.9510+24.2165 | 20:43:47.14 +24:12:29.7 (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 J310.9510+24.2165,2461125.8971,14.15,0.05,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
ATO J310.9510+24.2165 20260326.3971 14.15CV 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20.00sec_-14.90C_LIGHT_0634.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20.00sec_-15.00C_LIGHT_0635.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:43:47.14 +24:12:29.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_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 26.3971* 20 25 51.58 +20 14 02.3 14.0 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.8971,14.01,0.05,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 20260326.3971 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20.00sec_-14.90C_LIGHT_0634.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20.00sec_-15.00C_LIGHT_0635.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:51.58 +20:14:02.3 ;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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3971 2461125.8971 13.83 19:55:18.70 +20:35:33.1
58.49335 -3.94622 galactic Vul Second-epoch detections are separated by 2.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J298.8220+20.5918 | 19:55:18.70 +20:35:33.1 (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 J298.8220+20.5918,2461125.8971,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.8220+20.5918 20260326.3971 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20.00sec_-14.90C_LIGHT_0634.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20.00sec_-15.00C_LIGHT_0635.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:18.70 +20:35:33.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3971 2461125.8971 13.70 19:50:41.29 +18:29:32.3
56.12549 -4.08040 galactic Sge Second-epoch detections are separated by 3.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.6749+18.4852 | 19:50:41.29 +18:29:32.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.6749+18.4852,2461125.8971,13.70,0.05,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 J297.6749+18.4852 20260326.3971 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20.00sec_-14.90C_LIGHT_0634.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20.00sec_-15.00C_LIGHT_0635.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:50:41.29 +18:29:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_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,2461125.8971,13.04,0.05,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 20260326.3971 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20.00sec_-14.90C_LIGHT_0634.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20.00sec_-15.00C_LIGHT_0635.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:11.87 +22:19:37.1 ;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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3971 2461125.8971 13.62 20:38:31.83 +23:02:56.6
66.12514 -10.97454 galactic Vul Second-epoch detections are separated by 1.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J309.6539+23.0452 | 20:38:34.76 +23:02:43.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J309.6539+23.0452,2461125.8971,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J309.6539+23.0452 20260326.3971 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20.00sec_-14.90C_LIGHT_0634.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20.00sec_-15.00C_LIGHT_0635.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:38:31.83 +23:02:56.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_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 26.3971* 20 21 07.77 +19 19 34.9 14.2 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.8971,14.23,0.05,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 20260326.3971 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20.00sec_-14.90C_LIGHT_0634.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20.00sec_-15.00C_LIGHT_0635.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:21:07.77 +19:19:34.9 ;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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3971 2461125.8971 14.38 20:12:59.72 +22:48:05.7
62.55604 -6.26495 galactic Vul Second-epoch detections are separated by 0.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.2576+22.7951 | 20:13:01.82 +22:47:42.5 (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 J303.2576+22.7951,2461125.8971,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.2576+22.7951 20260326.3971 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20.00sec_-14.90C_LIGHT_0634.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20.00sec_-15.00C_LIGHT_0635.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:59.72 +22:48:05.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3971 2461125.8971 12.99 20:44:23.71 +20:40:02.0
64.97732 -13.47778 galactic Vul Second-epoch detections are separated by 3.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1814747450636884864 | 20:44:24.27 +20:39:36.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.462+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1814747450636884864,2461125.8971,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1814747450636884864 20260326.3971 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20.00sec_-14.90C_LIGHT_0634.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-02-Q2b1x1_043248_TTUQ2b1x1_30051_w3jODDOq/fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20.00sec_-15.00C_LIGHT_0635.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:23.71 +20:40:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-32-06_20_00sec_-15_00C_LIGHT_0635_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-26_04-31-19_20_00sec_-14_90C_LIGHT_0634_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3989 2461125.8989 13.79 18:52:03.81 -09:19:30.0
24.68738 -4.37490 galactic Sct Second-epoch detections are separated by 3.8" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J283.0152-09.3263 | 18:52:03.81 -09:19:30.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.872+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J283.0152-09.3263,2461125.8989,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.0152-09.3263 20260326.3989 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-33-48_20.00sec_-14.90C_LIGHT_0636.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20.00sec_-15.00C_LIGHT_0637.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:52:03.81 -09:19:30.0 ;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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_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_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3989 2461125.8989 13.53 18:52:16.43 -06:19:50.9
27.38716 -3.06719 galactic Sct Second-epoch detections are separated by 2.7" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J283.0715-06.3358 | 18:52:17.18 -06:20:09.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J283.0715-06.3358,2461125.8989,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.0715-06.3358 20260326.3989 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-33-48_20.00sec_-14.90C_LIGHT_0636.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20.00sec_-15.00C_LIGHT_0637.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:52:16.43 -06:19:50.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_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_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_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,2461125.8989,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.3989 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/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-33-48_20.00sec_-14.90C_LIGHT_0636.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20.00sec_-15.00C_LIGHT_0637.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:43:51.45 -05:52:12.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_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_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3989 2461125.8989 13.80 19:00:48.25 -06:03:12.8
28.59627 -4.83268 galactic Aql Second-epoch detections are separated by 3.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4253833092897398784 | 19:00:45.86 -06:02:54.9 (Gaia DR3) | ACV/roAm/ (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4253833092897398784,2461125.8989,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4253833092897398784 20260326.3989 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-03-19_05-32-39_20.00sec_-15.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-33-48_20.00sec_-14.90C_LIGHT_0636.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20.00sec_-15.00C_LIGHT_0637.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:00:48.25 -06:03:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_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_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.3989 2461125.8989 14.07 18:53:21.41 -12:37:31.9
21.86783 -6.13892 galactic Sct Second-epoch detections are separated by 4.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J283.3365-12.6257 | 18:53:21.41 -12:37:31.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.817+/-0.163 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J283.3365-12.6257,2461125.8989,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.3365-12.6257 20260326.3989 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-33-48_20.00sec_-14.90C_LIGHT_0636.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sct-01-Q2b1x1_043518_TTUQ2b1x1_24047_kfpBN0Lq/fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20.00sec_-15.00C_LIGHT_0637.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:53:21.41 -12:37:31.9 ;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_Sct-01-Q2b1x1_2026-03-19_05-32-39_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png resample_wcs_fd_Sct-01-Q2b1x1_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_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_2026-03-26_04-34-34_20_00sec_-15_00C_LIGHT_0637_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_2026-03-26_04-33-48_20_00sec_-14_90C_LIGHT_0636_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4004 2461125.9004 13.27 19:28:33.50 +07:31:39.2
43.89280 -4.73506 galactic Aql Second-epoch detections are separated by 1.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.1509+07.5249 | 19:28:33.50 +07:31:39.2 (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 J292.1509+07.5249,2461125.9004,13.27,0.05,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
ATO J292.1509+07.5249 20260326.4004 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Aql-02-Q2b1x1_043733_TTUQ2b1x1_13729_qwZqPBBV/fd_Aql-02-Q2b1x1_2026-03-26_04-35-55_20.00sec_-14.90C_LIGHT_0638.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_043733_TTUQ2b1x1_13729_qwZqPBBV/fd_Aql-02-Q2b1x1_2026-03-26_04-36-49_20.00sec_-15.00C_LIGHT_0639.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:33.50 +07:31:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-26_04-36-49_20_00sec_-15_00C_LIGHT_0639_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_2026-03-26_04-35-55_20_00sec_-14_90C_LIGHT_0638_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_2026-03-26_04-36-49_20_00sec_-15_00C_LIGHT_0639_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_2026-03-26_04-35-55_20_00sec_-14_90C_LIGHT_0638_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4004 2461125.9004 11.81 20:06:41.09 +05:09:35.0
46.44029 -14.17087 galactic Aql Second-epoch detections are separated by 0.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4247871678237022976 | 20:06:41.05 +05:09:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.618+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4247871678237022976,2461125.9004,11.81,0.05,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 4247871678237022976 20260326.4004 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Aql-02-Q2b1x1_043733_TTUQ2b1x1_13729_qwZqPBBV/fd_Aql-02-Q2b1x1_2026-03-26_04-35-55_20.00sec_-14.90C_LIGHT_0638.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_043733_TTUQ2b1x1_13729_qwZqPBBV/fd_Aql-02-Q2b1x1_2026-03-26_04-36-49_20.00sec_-15.00C_LIGHT_0639.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:06:41.09 +05:09:35.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-26_04-36-49_20_00sec_-15_00C_LIGHT_0639_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_2026-03-26_04-35-55_20_00sec_-14_90C_LIGHT_0638_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_2026-03-26_04-36-49_20_00sec_-15_00C_LIGHT_0639_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_2026-03-26_04-35-55_20_00sec_-14_90C_LIGHT_0638_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,2461125.9074,14.05,0.05,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
target 20260326.4074 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:43.93 +46:20:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4074 2461125.9074 13.30 21:55:39.38 +43:56:46.5
92.60156 -8.33265 galactic Cyg Second-epoch detections are separated by 1.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.9028+43.9373 | 21:55:39.38 +43:56:46.5 (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 J328.9028+43.9373,2461125.9074,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.9028+43.9373 20260326.4074 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:39.38 +43:56:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4074 2461125.9074 13.47 22:08:58.13 +46:23:21.8
95.98070 -7.80621 galactic Lac Second-epoch detections are separated by 1.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.2681+46.3903 | 22:09:00.96 +46:23:22.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.2681+46.3903,2461125.9074,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J332.2681+46.3903 20260326.4074 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:58.13 +46:23:21.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4074 2461125.9074 13.60 22:01:07.06 +48:31:14.3
96.18270 -5.30374 galactic Cyg Second-epoch detections are separated by 5.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.2749+48.5143 | 22:01:07.06 +48:31:14.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.2749+48.5143,2461125.9074,13.60,0.05,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
ATO J330.2749+48.5143 20260326.4074 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:01:07.06 +48:31:14.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4074 2461125.9074 13.65 21:43:26.79 +43:22:28.5
90.52013 -7.35740 galactic Cyg Second-epoch detections are separated by 2.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.8573+43.3692 | 21:43:29.60 +43:22:27.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.8573+43.3692,2461125.9074,13.65,0.05,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
ATO J325.8573+43.3692 20260326.4074 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/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:26.79 +43:22:28.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4074 2461125.9074 13.72 21:46:26.47 +44:15:59.4
91.51910 -7.03337 galactic Cyg Second-epoch detections are separated by 1.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.6042+44.2605 | 21:46:26.47 +44:15:59.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.6042+44.2605,2461125.9074,13.72,0.05,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
ATO J326.6042+44.2605 20260326.4074 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:46:26.47 +44:15:59.4 ;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_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4074 2461125.9074 13.63 21:28:54.93 +44:35:52.0
89.40555 -4.69326 galactic Cyg Second-epoch detections are separated by 1.2" 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 | ATO J322.2282+44.6106 | 21:28:54.93 +44:35:52.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.2282+44.6106,2461125.9074,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.2282+44.6106 20260326.4074 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:28:54.93 +44:35:52.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4074 2461125.9074 13.74 21:23:01.15 +47:06:38.7
90.42109 -2.17515 galactic Cyg Second-epoch detections are separated by 3.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.7527+47.1220 | 21:22:59.53 +47:07:13.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J320.7527+47.1220,2461125.9074,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J320.7527+47.1220 20260326.4074 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:01.15 +47:06:38.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4074 2461125.9074 13.83 21:38:39.29 +49:34:43.4
94.00606 -2.15074 galactic Cyg Second-epoch detections are separated by 7.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.6638+49.5826 | 21:38:36.16 +49:35:13.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.228+/- (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.6638+49.5826,2461125.9074,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.6638+49.5826 20260326.4074 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:38:39.29 +49:34:43.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4074 2461125.9074 14.04 21:48:44.24 +46:19:09.2
93.15982 -5.72262 galactic Cyg Second-epoch detections are separated by 4.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.1819+46.3185 | 21:48:44.24 +46:19:09.2 (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 J327.1819+46.3185,2461125.9074,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.1819+46.3185 20260326.4074 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20.00sec_-14.90C_LIGHT_0640.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_044733_TTUQ2b1x1_6063_oPicPAjl/fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20.00sec_-15.00C_LIGHT_0641.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:48:44.24 +46:19:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-46-55_20_00sec_-15_00C_LIGHT_0641_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_04-45-59_20_00sec_-14_90C_LIGHT_0640_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,2461125.9124,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4124 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-09-Q2b1x1_2025-12-26_19-09-20_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-09-Q2b1x1_045448_TTUQ2b1x1_2982_6r8UmBiF/fd_Cyg-09-Q2b1x1_2026-03-26_04-53-15_20.00sec_-14.90C_LIGHT_0642.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-09-Q2b1x1_045448_TTUQ2b1x1_2982_6r8UmBiF/fd_Cyg-09-Q2b1x1_2026-03-26_04-54-00_20.00sec_-15.00C_LIGHT_0643.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:10.11 +29:10:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-26_04-54-00_20_00sec_-15_00C_LIGHT_0643_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-26_04-53-15_20_00sec_-14_90C_LIGHT_0642_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-26_04-54-00_20_00sec_-15_00C_LIGHT_0643_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-09-Q2b1x1_2025-12-26_19-09-20_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Cyg-09-Q2b1x1_2026-03-26_04-53-15_20_00sec_-14_90C_LIGHT_0642_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4135 2461125.9135 13.64 18:30:14.94 -14:03:07.5
18.03660 -1.77688 galactic Sct Second-epoch detections are separated by 2.3" 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 J277.5523-14.0551 | 18:30:12.56 -14:03:18.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB 1963LS....C04....0N LS IV -14 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 J277.5523-14.0551,2461125.9135,13.64,0.05,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 J277.5523-14.0551 20260326.4135 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/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-02-Q2b1x1_045618_TTUQ2b1x1_15630_XdrAMM1a/fd_Sgr-02-Q2b1x1_2026-03-26_04-54-53_20.00sec_-14.90C_LIGHT_0644.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-02-Q2b1x1_045618_TTUQ2b1x1_15630_XdrAMM1a/fd_Sgr-02-Q2b1x1_2026-03-26_04-55-38_20.00sec_-15.00C_LIGHT_0645.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:30:14.94 -14:03:07.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-55-38_20_00sec_-15_00C_LIGHT_0645_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-54-53_20_00sec_-14_90C_LIGHT_0644_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-55-38_20_00sec_-15_00C_LIGHT_0645_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-54-53_20_00sec_-14_90C_LIGHT_0644_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4135 2461125.9135 13.32 18:16:15.88 -16:59:39.9
13.85794 -0.18119 galactic Sgr Second-epoch detections are separated by 8.1" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J274.0610-16.9942 | 18:16:14.66 -16:59:39.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J274.0610-16.9942,2461125.9135,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J274.0610-16.9942 20260326.4135 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-02-Q2b1x1_045618_TTUQ2b1x1_15630_XdrAMM1a/fd_Sgr-02-Q2b1x1_2026-03-26_04-54-53_20.00sec_-14.90C_LIGHT_0644.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-02-Q2b1x1_045618_TTUQ2b1x1_15630_XdrAMM1a/fd_Sgr-02-Q2b1x1_2026-03-26_04-55-38_20.00sec_-15.00C_LIGHT_0645.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:16:15.88 -16:59:39.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-55-38_20_00sec_-15_00C_LIGHT_0645_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-54-53_20_00sec_-14_90C_LIGHT_0644_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-55-38_20_00sec_-15_00C_LIGHT_0645_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-54-53_20_00sec_-14_90C_LIGHT_0644_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4135 2461125.9135 12.65 18:36:44.75 -17:13:51.2
15.92499 -4.62403 galactic Sgr Second-epoch detections are separated by 2.1" 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 J279.1958-17.2311 | 18:36:46.44 -17:13:50.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J279.1958-17.2311,2461125.9135,12.65,0.05,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
ATO J279.1958-17.2311 20260326.4135 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-02-Q2b1x1_045618_TTUQ2b1x1_15630_XdrAMM1a/fd_Sgr-02-Q2b1x1_2026-03-26_04-54-53_20.00sec_-14.90C_LIGHT_0644.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-02-Q2b1x1_045618_TTUQ2b1x1_15630_XdrAMM1a/fd_Sgr-02-Q2b1x1_2026-03-26_04-55-38_20.00sec_-15.00C_LIGHT_0645.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:36:44.75 -17:13:51.2 ;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_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-55-38_20_00sec_-15_00C_LIGHT_0645_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-54-53_20_00sec_-14_90C_LIGHT_0644_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-55-38_20_00sec_-15_00C_LIGHT_0645_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-26_04-54-53_20_00sec_-14_90C_LIGHT_0644_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4185 2461125.9185 13.75 19:25:33.98 +01:09:56.1
37.88814 -7.05020 galactic Aql Second-epoch detections are separated by 6.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.3981+01.1720 | 19:25:33.98 +01:09:56.1 (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 J291.3981+01.1720,2461125.9185,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J291.3981+01.1720 20260326.4185 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-03-20_05-22-14_20.00sec_-14.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20.00sec_-15.00C_LIGHT_0646.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20.00sec_-15.00C_LIGHT_0647.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:25:33.98 +01:09:56.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4185 2461125.9185 13.63 19:19:17.33 +02:03:56.3
37.96242 -5.24311 galactic Aql Second-epoch detections are separated by 7.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:19:17.33 +02:03:56.3 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9185,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4185 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-03-20_05-22-14_20.00sec_-14.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20.00sec_-15.00C_LIGHT_0646.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20.00sec_-15.00C_LIGHT_0647.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:19:17.33 +02:03:56.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4185 2461125.9185 13.65 19:23:44.92 -01:07:33.2
35.62562 -7.70038 galactic Aql Second-epoch detections are separated by 3.0" 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 J290.9346-01.1263 | 19:23:44.92 -01:07:33.2 (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 J290.9346-01.1263,2461125.9185,13.65,0.05,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
ATO J290.9346-01.1263 20260326.4185 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/Aql-04-Q2b1x1_2026-03-20_05-22-14_20.00sec_-14.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20.00sec_-15.00C_LIGHT_0646.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20.00sec_-15.00C_LIGHT_0647.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:23:44.92 -01:07:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4185 2461125.9185 13.51 19:16:49.03 -02:03:45.5
33.98898 -6.58644 galactic Aql Second-epoch detections are separated by 1.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J289.2034-02.0633 | 19:16:49.03 -02:03:45.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.585+/-0.053 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J289.2034-02.0633,2461125.9185,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.2034-02.0633 20260326.4185 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-03-20_05-22-14_20.00sec_-14.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20.00sec_-15.00C_LIGHT_0646.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20.00sec_-15.00C_LIGHT_0647.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:16:49.03 -02:03:45.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4185 2461125.9185 13.78 19:17:21.18 -00:21:25.9
35.57696 -5.92708 galactic Aql Second-epoch detections are separated by 4.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J289.3384-00.3522 | 19:17:21.18 -00:21:25.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J289.3384-00.3522,2461125.9185,13.78,0.05,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 J289.3384-00.3522 20260326.4185 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/Aql-04-Q2b1x1_2026-03-20_05-22-14_20.00sec_-14.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20.00sec_-15.00C_LIGHT_0646.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20.00sec_-15.00C_LIGHT_0647.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:17:21.18 -00:21:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4185 2461125.9185 13.71 19:16:49.99 +01:37:05.0
37.27974 -4.90484 galactic Aql Second-epoch detections are separated by 5.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J289.2170+01.6406 | 19:16:51.57 +01:37:40.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J289.2170+01.6406,2461125.9185,13.71,0.05,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
ATO J289.2170+01.6406 20260326.4185 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/Aql-04-Q2b1x1_2026-03-20_05-22-14_20.00sec_-14.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20.00sec_-15.00C_LIGHT_0646.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20.00sec_-15.00C_LIGHT_0647.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:16:49.99 +01:37:05.0 ;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_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4185 2461125.9185 13.75 19:24:10.58 -02:09:37.6
34.74548 -8.26785 galactic Aql Second-epoch detections are separated by 2.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.0377-02.1601 | 19:24:09.25 -02:08:57.2 (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 J291.0377-02.1601,2461125.9185,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J291.0377-02.1601 20260326.4185 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-03-20_05-22-14_20.00sec_-14.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20.00sec_-15.00C_LIGHT_0646.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20.00sec_-15.00C_LIGHT_0647.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:24:10.58 -02:09:37.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4185 2461125.9185 13.73 19:17:13.59 -01:10:07.1
34.83664 -6.26994 galactic Aql Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | NSVS 13997662 | 19:17:11.15 -01:10:17.2 (Gaia DR3) | SR (local) | 2458329.09600 (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13997662,2461125.9185,13.73,0.05,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
NSVS 13997662 20260326.4185 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/Aql-04-Q2b1x1_2026-03-20_05-22-14_20.00sec_-14.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20.00sec_-15.00C_LIGHT_0646.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20.00sec_-15.00C_LIGHT_0647.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:17:13.59 -01:10:07.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4185 2461125.9185 13.96 19:23:54.85 +01:55:16.9
38.37061 -6.33461 galactic Aql Second-epoch detections are separated by 3.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J290.9695+01.9196 | 19:23:54.85 +01:55:16.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J290.9695+01.9196,2461125.9185,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J290.9695+01.9196 20260326.4185 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-03-20_05-22-14_20.00sec_-14.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20.00sec_-15.00C_LIGHT_0646.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-04-Q2b1x1_050333_TTUQ2b1x1_25546_r85IJxx9/fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20.00sec_-15.00C_LIGHT_0647.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:23:54.85 +01:55:16.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-02-49_20_00sec_-15_00C_LIGHT_0647_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-04-Q2b1x1_2026-03-20_05-22-14_20_00sec_-14_90C_LIGHT_0450_fits__*pix.png resample_wcs_fd_Aql-04-Q2b1x1_2026-03-26_05-01-59_20_00sec_-15_00C_LIGHT_0646_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4196 2461125.9196 13.46 17:07:04.90 -32:51:14.0
352.13040 4.67006 galactic Sco Second-epoch detections are separated by 4.3" 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 | Large-amplitude variable Gaia DR2 5979990276015434752 | 17:07:04.90 -32:51:14.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 5979990276015434752,2461125.9196,13.46,0.05,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
Large-amplitude variable Gaia DR2 5979990276015434752 20260326.4196 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/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-03-Q2b1x1_050518_TTUQ2b1x1_7027_pr5vRd6y/fd_Sco-03-Q2b1x1_2026-03-26_05-03-41_20.00sec_-15.00C_LIGHT_0648.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-03-Q2b1x1_050518_TTUQ2b1x1_7027_pr5vRd6y/fd_Sco-03-Q2b1x1_2026-03-26_05-04-33_20.00sec_-15.00C_LIGHT_0649.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:07:04.90 -32:51:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-04-33_20_00sec_-15_00C_LIGHT_0649_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-03-41_20_00sec_-15_00C_LIGHT_0648_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-04-33_20_00sec_-15_00C_LIGHT_0649_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-03-41_20_00sec_-15_00C_LIGHT_0648_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4196 2461125.9196 13.55 16:51:13.38 -36:46:06.1
347.02527 4.82446 galactic Sco Second-epoch detections are separated by 4.1" 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 | 16:51:13.38 -36:46:06.1 (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,2461125.9196,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4196 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-03-Q2b1x1_050518_TTUQ2b1x1_7027_pr5vRd6y/fd_Sco-03-Q2b1x1_2026-03-26_05-03-41_20.00sec_-15.00C_LIGHT_0648.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-03-Q2b1x1_050518_TTUQ2b1x1_7027_pr5vRd6y/fd_Sco-03-Q2b1x1_2026-03-26_05-04-33_20.00sec_-15.00C_LIGHT_0649.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:51:13.38 -36:46:06.1 ;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_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-04-33_20_00sec_-15_00C_LIGHT_0649_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-03-41_20_00sec_-15_00C_LIGHT_0648_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-04-33_20_00sec_-15_00C_LIGHT_0649_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-03-41_20_00sec_-15_00C_LIGHT_0648_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4196 2461125.9196 13.47 17:00:28.33 -30:06:53.4
353.47498 7.44491 galactic Oph Second-epoch detections are separated by 1.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:00:28.33 -30:06:53.4 (user input) | T | P | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9196,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4196 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-03-Q2b1x1_050518_TTUQ2b1x1_7027_pr5vRd6y/fd_Sco-03-Q2b1x1_2026-03-26_05-03-41_20.00sec_-15.00C_LIGHT_0648.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-03-Q2b1x1_050518_TTUQ2b1x1_7027_pr5vRd6y/fd_Sco-03-Q2b1x1_2026-03-26_05-04-33_20.00sec_-15.00C_LIGHT_0649.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:00:28.33 -30:06:53.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-04-33_20_00sec_-15_00C_LIGHT_0649_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-03-41_20_00sec_-15_00C_LIGHT_0648_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-04-33_20_00sec_-15_00C_LIGHT_0649_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Sco-03-Q2b1x1_2026-03-26_05-03-41_20_00sec_-15_00C_LIGHT_0648_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4209 2461125.9209 11.62 20:04:12.71 +12:50:08.4
52.89883 -9.76660 galactic Aql Second-epoch detections are separated by 1.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J301.0426+12.8341 | 20:04:12.31 +12:50:06.2 (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 J301.0426+12.8341,2461125.9209,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J301.0426+12.8341 20260326.4209 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:04:12.71 +12:50:08.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_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,2461125.9209,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4209 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:03:03.85 +16:47:54.0 ;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_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_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,2461125.9209,13.65,0.05,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 20260326.4209 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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:58:01.53 +17:20:11.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_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 26.4209* 20 49 10.26 +15 30 31.3 14.0 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9209,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4209 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:49:10.26 +15:30:31.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_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,2461125.9209,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4209 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:00:23.29 +17:40:17.5 ;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_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4209 2461125.9209 13.70 20:17:52.23 +09:53:02.1
52.08933 -14.15871 galactic Del Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1753421949080850304 | 20:17:49.85 +09:53:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.4209* 20 17 52.23 +09 53 02.1 13.7 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1753421949080850304,2461125.9209,13.70,0.05,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
Gaia DR3 1753421949080850304 20260326.4209 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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:17:52.23 +09:53:02.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4209 2461125.9209 13.96 20:40:31.61 +14:24:00.8
59.13663 -16.35551 galactic Del Second-epoch detections are separated by 2.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1762348609106144256 | 20:40:33.24 +14:24:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.4209* 20 40 31.61 +14 24 00.8 14.0 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1762348609106144256,2461125.9209,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1762348609106144256 20260326.4209 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:40:31.61 +14:24:00.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_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,2461125.9209,14.09,0.05,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 20260326.4209 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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:06:25.23 +13:36:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_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,2461125.9209,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4209 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:02.30 +13:18:43.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4209 2461125.9209 12.36 20:42:16.08 +17:20:00.6
61.88422 -15.02036 galactic Del Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1811457535748681344 | 20:42:16.04 +17:19:59.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.152+/-0.029 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.4209* 20 42 16.08 +17 20 00.6 12.4 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1811457535748681344,2461125.9209,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1811457535748681344 20260326.4209 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20.00sec_-15.00C_LIGHT_0650.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-01-Q2b1x1_050703_TTUQ2b1x1_2118_eeuH0XLd/fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20.00sec_-15.00C_LIGHT_0651.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:42:16.08 +17:20:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-06-18_20_00sec_-15_00C_LIGHT_0651_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-26_05-05-27_20_00sec_-15_00C_LIGHT_0650_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4264 2461125.9264 10.71 18:02:30.57 -23:00:56.6
7.02594 -0.27092 galactic Sgr Second-epoch detections are separated by 0.1" 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 | Gaia DR3 4069268796137510400 | 18:02:30.69 -23:00:42.1 (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 4069268796137510400,2461125.9264,10.71,0.05,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
Gaia DR3 4069268796137510400 20260326.4264 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-04-Q2b1x1_051503_TTUQ2b1x1_14150_G65nsL9Q/fd_Sgr-04-Q2b1x1_2026-03-26_05-13-30_20.00sec_-14.90C_LIGHT_0652.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-04-Q2b1x1_051503_TTUQ2b1x1_14150_G65nsL9Q/fd_Sgr-04-Q2b1x1_2026-03-26_05-14-16_20.00sec_-15.00C_LIGHT_0653.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:02:30.57 -23:00:56.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-26_05-14-16_20_00sec_-15_00C_LIGHT_0653_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-26_05-13-30_20_00sec_-14_90C_LIGHT_0652_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-26_05-14-16_20_00sec_-15_00C_LIGHT_0653_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-26_05-13-30_20_00sec_-14_90C_LIGHT_0652_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4264 2461125.9264 13.12 18:02:36.39 -23:53:32.0
6.27445 -0.72265 galactic Sgr Second-epoch detections are separated by 5.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J270.6563-23.8949 | 18:02:34.88 -23:53:23.5 (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 J270.6563-23.8949,2461125.9264,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J270.6563-23.8949 20260326.4264 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-04-Q2b1x1_051503_TTUQ2b1x1_14150_G65nsL9Q/fd_Sgr-04-Q2b1x1_2026-03-26_05-13-30_20.00sec_-14.90C_LIGHT_0652.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-04-Q2b1x1_051503_TTUQ2b1x1_14150_G65nsL9Q/fd_Sgr-04-Q2b1x1_2026-03-26_05-14-16_20.00sec_-15.00C_LIGHT_0653.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:02:36.39 -23:53:32.0 ;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_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-26_05-14-16_20_00sec_-15_00C_LIGHT_0653_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-26_05-13-30_20_00sec_-14_90C_LIGHT_0652_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-26_05-14-16_20_00sec_-15_00C_LIGHT_0653_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-26_05-13-30_20_00sec_-14_90C_LIGHT_0652_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4291 2461125.9291 13.50 22:16:54.79 +50:07:07.7
99.21891 -5.50177 galactic Lac Second-epoch detections are separated by 3.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.2288+50.1216 | 22:16:54.79 +50:07:07.7 (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 J334.2288+50.1216,2461125.9291,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.2288+50.1216 20260326.4291 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-26_19-35-41_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20.00sec_-14.90C_LIGHT_0654.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20.00sec_-15.00C_LIGHT_0655.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:54.79 +50:07:07.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4291 2461125.9291 13.60 22:09:32.87 +54:21:00.5
100.69638 -1.37888 galactic Cep Second-epoch detections are separated by 3.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.3951+54.3440 | 22:09:32.87 +54:21:00.5 (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 J332.3951+54.3440,2461125.9291,13.60,0.05,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
ATO J332.3951+54.3440 20260326.4291 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-26_19-35-41_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20.00sec_-14.90C_LIGHT_0654.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20.00sec_-15.00C_LIGHT_0655.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:32.87 +54:21:00.5 ;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_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4291 2461125.9291 12.26 22:50:39.48 +51:07:48.6
104.37598 -7.33774 galactic Lac Second-epoch detections are separated by 2.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J342.6854+51.1288 | 22:50:41.12 +51:07:57.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J342.6854+51.1288,2461125.9291,12.26,0.05,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
ATO J342.6854+51.1288 20260326.4291 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-26_19-35-41_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20.00sec_-14.90C_LIGHT_0654.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20.00sec_-15.00C_LIGHT_0655.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:50:39.48 +51:07:48.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4291 2461125.9291 13.45 22:09:52.31 +52:04:15.0
99.41811 -3.26738 galactic Lac Second-epoch detections are separated by 3.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J332.4719+52.0775 | 22:09:52.31 +52:04:15.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J332.4719+52.0775,2461125.9291,13.45,0.05,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 J332.4719+52.0775 20260326.4291 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/Lac-01-Q2b1x1_2025-12-26_19-35-41_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20.00sec_-14.90C_LIGHT_0654.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20.00sec_-15.00C_LIGHT_0655.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:52.31 +52:04:15.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4291 2461125.9291 13.69 22:20:01.74 +53:07:23.3
101.28816 -3.26494 galactic Lac Second-epoch detections are separated by 3.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2004672416306923648 | 22:20:00.75 +53:06:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2III 1955ApJS....2...75M LF 4 +52 386
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2004672416306923648,2461125.9291,13.69,0.05,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
Gaia DR3 2004672416306923648 20260326.4291 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/Lac-01-Q2b1x1_2025-12-26_19-35-41_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20.00sec_-14.90C_LIGHT_0654.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20.00sec_-15.00C_LIGHT_0655.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:20:01.74 +53:07:23.3 ;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_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_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,2461125.9291,13.69,0.05,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
target 20260326.4291 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/Lac-01-Q2b1x1_2025-12-26_19-35-41_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20.00sec_-14.90C_LIGHT_0654.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20.00sec_-15.00C_LIGHT_0655.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:39:42.14 +53:41:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4291 2461125.9291 13.82 22:47:48.84 +52:58:02.8
104.82592 -5.50286 galactic Lac Second-epoch detections are separated by 2.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J341.9586+52.9701 | 22:47:47.86 +52:58:33.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M3 1961JO.....44..247P GSC 3984-2188
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J341.9586+52.9701,2461125.9291,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J341.9586+52.9701 20260326.4291 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-26_19-35-41_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20.00sec_-14.90C_LIGHT_0654.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20.00sec_-15.00C_LIGHT_0655.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:47:48.84 +52:58:02.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4291 2461125.9291 13.97 22:31:38.38 +51:15:34.1
101.81167 -5.78787 galactic Lac Second-epoch detections are separated by 1.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J337.9111+51.2612 | 22:31:38.38 +51:15:34.1 (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 J337.9111+51.2612,2461125.9291,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J337.9111+51.2612 20260326.4291 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-01-Q2b1x1_2025-12-26_19-35-41_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20.00sec_-14.90C_LIGHT_0654.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-01-Q2b1x1_051848_TTUQ2b1x1_2916_toBRcV0q/fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20.00sec_-15.00C_LIGHT_0655.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:31:38.38 +51:15:34.1 ;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_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-18-04_20_00sec_-15_00C_LIGHT_0655_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-01-Q2b1x1_2025-12-26_19-35-41_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Lac-01-Q2b1x1_2026-03-26_05-17-15_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4321 2461125.9321 14.03 21:20:43.53 +38:32:14.1
84.02564 -7.93114 galactic Cyg Second-epoch detections are separated by 2.3" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.1791+38.5373 | 21:20:43.53 +38:32:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.029+/-0.189 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J320.1791+38.5373,2461125.9321,14.03,0.05,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
ATO J320.1791+38.5373 20260326.4321 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/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-07-Q2b1x1_052318_TTUQ2b1x1_10253_ywCQDXcv/fd_Cyg-07-Q2b1x1_2026-03-26_05-21-45_20.00sec_-14.90C_LIGHT_0656.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-07-Q2b1x1_052318_TTUQ2b1x1_10253_ywCQDXcv/fd_Cyg-07-Q2b1x1_2026-03-26_05-22-29_20.00sec_-14.90C_LIGHT_0657.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:43.53 +38:32:14.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-22-29_20_00sec_-14_90C_LIGHT_0657_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-21-45_20_00sec_-14_90C_LIGHT_0656_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-22-29_20_00sec_-14_90C_LIGHT_0657_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-21-45_20_00sec_-14_90C_LIGHT_0656_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4321 2461125.9321 13.57 22:06:28.71 +38:42:59.9
90.96504 -13.70742 galactic Lac Second-epoch detections are separated by 1.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1955878942113735168 | 22:06:27.77 +38:42:36.2 (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 1955878942113735168,2461125.9321,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1955878942113735168 20260326.4321 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-07-Q2b1x1_052318_TTUQ2b1x1_10253_ywCQDXcv/fd_Cyg-07-Q2b1x1_2026-03-26_05-21-45_20.00sec_-14.90C_LIGHT_0656.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-07-Q2b1x1_052318_TTUQ2b1x1_10253_ywCQDXcv/fd_Cyg-07-Q2b1x1_2026-03-26_05-22-29_20.00sec_-14.90C_LIGHT_0657.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:06:28.71 +38:42:59.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-22-29_20_00sec_-14_90C_LIGHT_0657_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-21-45_20_00sec_-14_90C_LIGHT_0656_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-22-29_20_00sec_-14_90C_LIGHT_0657_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-21-45_20_00sec_-14_90C_LIGHT_0656_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4321 2461125.9321 13.73 21:34:12.48 +39:03:26.1
86.29238 -9.39715 galactic Cyg Second-epoch detections are separated by 2.5" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J213414.64+390328.0 | 21:34:14.70 +39:03:29.1 (Gaia DR3) | YSO (local) | d (local) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213414.64+390328.0,2461125.9321,13.73,0.05,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
ASASSN-V J213414.64+390328.0 20260326.4321 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/Cyg-07-Q2b1x1_2025-12-26_19-22-56_20.00sec_-15.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-07-Q2b1x1_052318_TTUQ2b1x1_10253_ywCQDXcv/fd_Cyg-07-Q2b1x1_2026-03-26_05-21-45_20.00sec_-14.90C_LIGHT_0656.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-07-Q2b1x1_052318_TTUQ2b1x1_10253_ywCQDXcv/fd_Cyg-07-Q2b1x1_2026-03-26_05-22-29_20.00sec_-14.90C_LIGHT_0657.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:12.48 +39:03:26.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-22-29_20_00sec_-14_90C_LIGHT_0657_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-21-45_20_00sec_-14_90C_LIGHT_0656_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-22-29_20_00sec_-14_90C_LIGHT_0657_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q2b1x1_2025-12-26_19-22-56_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png resample_wcs_fd_Cyg-07-Q2b1x1_2026-03-26_05-21-45_20_00sec_-14_90C_LIGHT_0656_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4345 2461125.9345 13.77 19:20:06.32 -05:47:14.4
31.00882 -9.00079 galactic Aql Second-epoch detections are separated by 4.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4211110125441222528 | 19:20:04.40 -05:46:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4211110125441222528,2461125.9345,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4211110125441222528 20260326.4345 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-06-Q2b1x1_2026-03-19_06-31-15_20.00sec_-15.00C_LIGHT_0217.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-06-Q2b1x1_052648_TTUQ2b1x1_23383_HVHdbn5t/fd_Aql-06-Q2b1x1_2026-03-26_05-25-11_20.00sec_-15.00C_LIGHT_0658.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-06-Q2b1x1_052648_TTUQ2b1x1_23383_HVHdbn5t/fd_Aql-06-Q2b1x1_2026-03-26_05-25-58_20.00sec_-15.00C_LIGHT_0659.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:20:06.32 -05:47:14.4 ;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-06-Q2b1x1_2026-03-19_06-31-15_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png resample_wcs_fd_Aql-06-Q2b1x1_2026-03-26_05-25-58_20_00sec_-15_00C_LIGHT_0659_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-06-Q2b1x1_2026-03-19_06-31-15_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png resample_wcs_fd_Aql-06-Q2b1x1_2026-03-26_05-25-11_20_00sec_-15_00C_LIGHT_0658_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-06-Q2b1x1_2026-03-19_06-31-15_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png resample_wcs_fd_Aql-06-Q2b1x1_2026-03-26_05-25-58_20_00sec_-15_00C_LIGHT_0659_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-06-Q2b1x1_2026-03-19_06-31-15_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png resample_wcs_fd_Aql-06-Q2b1x1_2026-03-26_05-25-11_20_00sec_-15_00C_LIGHT_0658_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4368 2461125.9368 13.45 20:08:23.93 +09:53:07.0
50.85399 -12.15997 galactic Aql Second-epoch detections are separated by 1.7" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J302.0969+09.8853 | 20:08:23.93 +09:53:07.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.0969+09.8853,2461125.9368,13.45,0.05,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 J302.0969+09.8853 20260326.4368 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/Del-02-Q2b1x1_2026-03-20_05-51-54_20.00sec_-14.90C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-02-Q2b1x1_052951_TTUQ2b1x1_1621_wlHwIzmP/fd_Del-02-Q2b1x1_2026-03-26_05-28-25_20.00sec_-15.00C_LIGHT_0662.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-02-Q2b1x1_052951_TTUQ2b1x1_1621_wlHwIzmP/fd_Del-02-Q2b1x1_2026-03-26_05-29-13_20.00sec_-14.90C_LIGHT_0663.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:08:23.93 +09:53:07.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-02-Q2b1x1_2026-03-20_05-51-54_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png resample_wcs_fd_Del-02-Q2b1x1_2026-03-26_05-29-13_20_00sec_-14_90C_LIGHT_0663_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-02-Q2b1x1_2026-03-20_05-51-54_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png resample_wcs_fd_Del-02-Q2b1x1_2026-03-26_05-28-25_20_00sec_-15_00C_LIGHT_0662_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-02-Q2b1x1_2026-03-20_05-51-54_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png resample_wcs_fd_Del-02-Q2b1x1_2026-03-26_05-29-13_20_00sec_-14_90C_LIGHT_0663_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-02-Q2b1x1_2026-03-20_05-51-54_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png resample_wcs_fd_Del-02-Q2b1x1_2026-03-26_05-28-25_20_00sec_-15_00C_LIGHT_0662_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,2461125.9368,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4368 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-03-20_05-51-54_20.00sec_-14.90C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-02-Q2b1x1_052951_TTUQ2b1x1_1621_wlHwIzmP/fd_Del-02-Q2b1x1_2026-03-26_05-28-25_20.00sec_-15.00C_LIGHT_0662.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Del-02-Q2b1x1_052951_TTUQ2b1x1_1621_wlHwIzmP/fd_Del-02-Q2b1x1_2026-03-26_05-29-13_20.00sec_-14.90C_LIGHT_0663.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:01.39 +08:37:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-02-Q2b1x1_2026-03-20_05-51-54_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png resample_wcs_fd_Del-02-Q2b1x1_2026-03-26_05-29-13_20_00sec_-14_90C_LIGHT_0663_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-02-Q2b1x1_2026-03-20_05-51-54_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png resample_wcs_fd_Del-02-Q2b1x1_2026-03-26_05-28-25_20_00sec_-15_00C_LIGHT_0662_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-02-Q2b1x1_2026-03-20_05-51-54_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png resample_wcs_fd_Del-02-Q2b1x1_2026-03-26_05-29-13_20_00sec_-14_90C_LIGHT_0663_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-02-Q2b1x1_2026-03-20_05-51-54_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png resample_wcs_fd_Del-02-Q2b1x1_2026-03-26_05-28-25_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4550 2461125.9550 13.86 19:29:15.28 -13:58:00.6
24.48696 -14.59132 galactic Sgr Second-epoch detections are separated by 2.7" 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 J292.3142-13.9668 | 19:29:15.28 -13:58:00.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.821+/-0.076 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.3142-13.9668,2461125.9550,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.3142-13.9668 20260326.4550 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:15.28 -13:58:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_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,2461125.9550,13.46,0.05,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 20260326.4550 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/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:46:32.98 -18:53:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4572 2461125.9572 14.46 22:36:52.36 +46:21:19.1
100.05155 -10.45226 galactic Lac Second-epoch detections are separated by 8.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J339.2017+46.3416 | 22:36:48.27 +46:20:59.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.717+/-0.083 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J339.2017+46.3416,2461125.9572,14.46,0.05,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 J339.2017+46.3416 20260326.4572 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lac-02-Q2b1x1_2025-12-26_19-37-28_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-02-Q2b1x1_055918_TTUQ2b1x1_601_NvzJqMHI/fd_Lac-02-Q2b1x1_2026-03-26_05-57-49_20.00sec_-14.90C_LIGHT_0669.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Lac-02-Q2b1x1_055918_TTUQ2b1x1_601_NvzJqMHI/fd_Lac-02-Q2b1x1_2026-03-26_05-58-35_20.00sec_-14.90C_LIGHT_0670.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:36:52.36 +46:21:19.1 ;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_Lac-02-Q2b1x1_2025-12-26_19-37-28_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Lac-02-Q2b1x1_2026-03-26_05-58-35_20_00sec_-14_90C_LIGHT_0670_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-02-Q2b1x1_2025-12-26_19-37-28_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Lac-02-Q2b1x1_2026-03-26_05-57-49_20_00sec_-14_90C_LIGHT_0669_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-02-Q2b1x1_2025-12-26_19-37-28_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Lac-02-Q2b1x1_2026-03-26_05-58-35_20_00sec_-14_90C_LIGHT_0670_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-02-Q2b1x1_2025-12-26_19-37-28_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Lac-02-Q2b1x1_2026-03-26_05-57-49_20_00sec_-14_90C_LIGHT_0669_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 26.4583* 20 57 57.59 +14 33 19.2 14.4 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9583,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4583 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-08-Q2b1x1_060105_TTUQ2b1x1_30721_D3SiiEZ8/fd_Peg-08-Q2b1x1_2026-03-26_05-59-27_20.00sec_-15.00C_LIGHT_0671.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-08-Q2b1x1_060105_TTUQ2b1x1_30721_D3SiiEZ8/fd_Peg-08-Q2b1x1_2026-03-26_06-00-15_20.00sec_-14.90C_LIGHT_0672.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:57:57.59 +14:33:19.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20_00sec_-14_90C_LIGHT_0000_fits__*pix.png resample_wcs_fd_Peg-08-Q2b1x1_2026-03-26_06-00-15_20_00sec_-14_90C_LIGHT_0672_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20_00sec_-14_90C_LIGHT_0000_fits__*pix.png resample_wcs_fd_Peg-08-Q2b1x1_2026-03-26_05-59-27_20_00sec_-15_00C_LIGHT_0671_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20_00sec_-14_90C_LIGHT_0000_fits__*pix.png resample_wcs_fd_Peg-08-Q2b1x1_2026-03-26_06-00-15_20_00sec_-14_90C_LIGHT_0672_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20_00sec_-14_90C_LIGHT_0000_fits__*pix.png resample_wcs_fd_Peg-08-Q2b1x1_2026-03-26_05-59-27_20_00sec_-15_00C_LIGHT_0671_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,2461125.9595,14.03,0.05,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
target 20260326.4595 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/Aql-05-Q2b1x1_2026-03-20_06-19-14_20.00sec_-14.90C_LIGHT_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-05-Q2b1x1_060308_TTUQ2b1x1_7814_WgXgrOWc/fd_Aql-05-Q2b1x1_2026-03-26_06-01-03_20.00sec_-15.00C_LIGHT_0673.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-05-Q2b1x1_060308_TTUQ2b1x1_7814_WgXgrOWc/fd_Aql-05-Q2b1x1_2026-03-26_06-01-51_20.00sec_-15.00C_LIGHT_0674.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:26:20.13 -04:27:45.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-05-Q2b1x1_2026-03-20_06-19-14_20_00sec_-14_90C_LIGHT_0475_fits__*pix.png resample_wcs_fd_Aql-05-Q2b1x1_2026-03-26_06-01-51_20_00sec_-15_00C_LIGHT_0674_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-05-Q2b1x1_2026-03-20_06-19-14_20_00sec_-14_90C_LIGHT_0475_fits__*pix.png resample_wcs_fd_Aql-05-Q2b1x1_2026-03-26_06-01-03_20_00sec_-15_00C_LIGHT_0673_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-05-Q2b1x1_2026-03-20_06-19-14_20_00sec_-14_90C_LIGHT_0475_fits__*pix.png resample_wcs_fd_Aql-05-Q2b1x1_2026-03-26_06-01-51_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-05-Q2b1x1_2026-03-20_06-19-14_20_00sec_-14_90C_LIGHT_0475_fits__*pix.png resample_wcs_fd_Aql-05-Q2b1x1_2026-03-26_06-01-03_20_00sec_-15_00C_LIGHT_0673_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4641 2461125.9641 11.30 20:29:15.74 +55:01:45.4
91.01028 9.35046 galactic Cyg Second-epoch detections are separated by 2.4" 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 | ASASSN-V J202913.08+550159.1 | 20:29:13.10 +55:01:58.4 (Gaia DR3) | SR (local) | 68.200000000000 (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202913.08+550159.1,2461125.9641,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202913.08+550159.1 20260326.4641 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20.00sec_-14.90C_LIGHT_0677.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20.00sec_-15.00C_LIGHT_0678.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:29:15.74 +55:01:45.4 ;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-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_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,2461125.9641,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4641 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/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20.00sec_-14.90C_LIGHT_0677.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20.00sec_-15.00C_LIGHT_0678.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:50:00.16 +52:43:07.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4641 2461125.9641 13.83 21:35:08.84 +50:02:59.1
93.89985 -1.42222 galactic Cyg Second-epoch detections are separated by 5.6" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.7860+50.0543 | 21:35:08.84 +50:02:59.1 (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 J323.7860+50.0543,2461125.9641,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.7860+50.0543 20260326.4641 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20.00sec_-14.90C_LIGHT_0677.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20.00sec_-15.00C_LIGHT_0678.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:08.84 +50:02:59.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4641 2461125.9641 14.29 20:48:31.99 +50:34:19.5
89.17996 4.34839 galactic Cyg Second-epoch detections are separated by 1.6" 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 J312.1345+50.5653 | 20:48:31.99 +50:34:19.5 (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 J312.1345+50.5653,2461125.9641,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.1345+50.5653 20260326.4641 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20.00sec_-14.90C_LIGHT_0677.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20.00sec_-15.00C_LIGHT_0678.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:48:31.99 +50:34:19.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4641 2461125.9641 14.36 20:35:14.26 +52:32:47.3
89.48675 7.18955 galactic Cyg Second-epoch detections are separated by 5.9" 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 | ATO J308.8156+52.5350 | 20:35:15.75 +52:32:06.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J308.8156+52.5350,2461125.9641,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J308.8156+52.5350 20260326.4641 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-26_19-15-01_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20.00sec_-14.90C_LIGHT_0677.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-02-Q2b1x1_060918_TTUQ2b1x1_26677_Pa0T8Ye6/fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20.00sec_-15.00C_LIGHT_0678.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:35:14.26 +52:32:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-08-26_20_00sec_-15_00C_LIGHT_0678_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-26_19-15-01_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-26_06-07-42_20_00sec_-14_90C_LIGHT_0677_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,2461125.9653,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4653 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:54.31 +42:56:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4653 2461125.9653 14.24 19:58:20.32 +48:16:58.8
82.63821 9.78363 galactic Cyg Second-epoch detections are separated by 6.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.5888+48.2801 | 19:58:20.32 +48:16:58.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5888+48.2801,2461125.9653,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5888+48.2801 20260326.4653 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:58:20.32 +48:16:58.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4653 2461125.9653 14.01 20:06:34.79 +41:50:12.7
77.83734 5.19909 galactic Cyg Second-epoch detections are separated by 4.9" 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 | Gaia DR3 2074857645125284992 | 20:06:35.53 +41:50:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2074857645125284992,2461125.9653,14.01,0.05,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 2074857645125284992 20260326.4653 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:06:34.79 +41:50:12.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4653 2461125.9653 12.77 20:54:09.72 +45:07:49.9
85.57760 0.15937 galactic Cyg Second-epoch detections are separated by 3.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.5485+45.1328 | 20:54:13.91 +45:07:46.7 (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 J313.5485+45.1328,2461125.9653,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.5485+45.1328 20260326.4653 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:54:09.72 +45:07:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4653 2461125.9653 13.88 20:11:56.23 +46:22:50.3
82.21145 6.82618 galactic Cyg Second-epoch detections are separated by 8.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J302.9910+46.3779 | 20:11:56.47 +46:23:23.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.9910+46.3779,2461125.9653,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J302.9910+46.3779 20260326.4653 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:11:56.23 +46:22:50.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_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,2461125.9653,14.20,0.05,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 20260326.4653 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:58:21.99 +45:30:43.6 ;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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4653 2461125.9653 14.38 20:53:53.56 +45:33:10.4
85.87056 0.46727 galactic Cyg Second-epoch detections are separated by 2.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.4733+45.5542 | 20:53:53.56 +45:33:10.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.4733+45.5542,2461125.9653,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.4733+45.5542 20260326.4653 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:53:53.56 +45:33:10.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4653 2461125.9653 14.29 19:54:20.45 +45:06:32.8
79.50609 8.78937 galactic Cyg Second-epoch detections are separated by 2.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2079211058327731968 | 19:54:21.09 +45:07:05.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2079211058327731968,2461125.9653,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2079211058327731968 20260326.4653 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:20.45 +45:06:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4653 2461125.9653 14.34 19:52:08.48 +42:55:49.9
77.39726 8.04726 galactic Cyg Second-epoch detections are separated by 0.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:52:08.48 +42:55:49.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9653,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4653 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:52:08.48 +42:55:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4653 2461125.9653 14.45 20:22:45.37 +48:32:00.4
85.03478 6.49009 galactic Cyg Second-epoch detections are separated by 5.0" 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 | ATO J305.6912+48.5332 | 20:22:45.37 +48:32:00.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J305.6912+48.5332,2461125.9653,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J305.6912+48.5332 20260326.4653 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20.00sec_-15.00C_LIGHT_0679.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-03-Q2b1x1_061103_TTUQ2b1x1_31128_XA4PO5sW/fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20.00sec_-15.00C_LIGHT_0680.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:22:45.37 +48:32:00.4 ;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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-10-16_20_00sec_-15_00C_LIGHT_0680_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-26_06-09-29_20_00sec_-15_00C_LIGHT_0679_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.37 20:16:36.53 +39:32:28.0
76.94901 2.35349 galactic Cyg Second-epoch detections are separated by 1.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.1466+39.5346 | 20:16:36.53 +39:32:28.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.250+/-0.157 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.1466+39.5346,2461125.9688,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.1466+39.5346 20260326.4688 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:36.53 +39:32:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.37 21:00:59.88 +34:36:20.7
78.40075 -7.66823 galactic Cyg Second-epoch detections are separated by 1.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2541+34.6011 | 21:00:59.88 +34:36:20.7 (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 J315.2541+34.6011,2461125.9688,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2541+34.6011 20260326.4688 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:59.88 +34:36:20.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.23 20:51:55.87 +37:28:46.7
79.42522 -4.41572 galactic Cyg Second-epoch detections are separated by 2.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.9916+37.4783 | 20:51:55.87 +37:28:46.7 (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 J312.9916+37.4783,2461125.9688,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.9916+37.4783 20260326.4688 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:51:55.87 +37:28:46.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 13.37 20:55:04.02 +35:22:54.2
78.20675 -6.23979 galactic Cyg Second-epoch detections are separated by 6.5" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1869678158220296448 | 20:55:06.45 +35:22:38.0 (Gaia DR3) | BCEP (local) | (local) | Gaia3var=VARIABLE SpType: B6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1869678158220296448,2461125.9688,13.37,0.05,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
Gaia DR3 1869678158220296448 20260326.4688 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:55:04.02 +35:22:54.2 ;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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 13.18 20:53:27.59 +39:21:09.2
81.06247 -3.45159 galactic Cyg Second-epoch detections are separated by 1.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.3774+39.3540 | 20:53:27.59 +39:21:09.2 (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 J313.3774+39.3540,2461125.9688,13.18,0.05,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
ATO J313.3774+39.3540 20260326.4688 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:53:27.59 +39:21:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 13.41 21:07:35.08 +38:51:48.9
82.49490 -5.84071 galactic Cyg Second-epoch detections are separated by 4.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.8944+38.8640 | 21:07:35.08 +38:51:48.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J316.8944+38.8640,2461125.9688,13.41,0.05,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
ATO J316.8944+38.8640 20260326.4688 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:07:35.08 +38:51:48.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.19 21:00:46.27 +33:53:57.8
77.82874 -8.09262 galactic Cyg Second-epoch detections are separated by 3.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1901+33.9002 | 21:00:46.27 +33:53:57.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1901+33.9002,2461125.9688,14.19,0.05,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 J315.1901+33.9002 20260326.4688 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:46.27 +33:53:57.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.21 20:44:45.54 +35:25:21.7
76.91089 -4.58165 galactic Cyg Second-epoch detections are separated by 1.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.1793+35.4270 | 20:44:45.54 +35:25:21.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.1793+35.4270,2461125.9688,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.1793+35.4270 20260326.4688 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:45.54 +35:25:21.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.35 21:01:59.28 +38:08:24.8
81.22047 -5.50330 galactic Cyg Second-epoch detections are separated by 3.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5027+38.1461 | 21:01:59.28 +38:08:24.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5027+38.1461,2461125.9688,14.35,0.05,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
ATO J315.5027+38.1461 20260326.4688 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:59.28 +38:08:24.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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,2461125.9688,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4688 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:50:16.45 +35:27:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.33 20:46:32.96 +38:44:19.0
79.73643 -2.80043 galactic Cyg Second-epoch detections are separated by 2.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.6376+38.7353 | 20:46:32.96 +38:44:19.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.6376+38.7353,2461125.9688,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.6376+38.7353 20260326.4688 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:46:32.96 +38:44:19.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.38 20:58:04.10 +38:34:01.4
81.04010 -4.64283 galactic Cyg Second-epoch detections are separated by 5.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5319+38.5720 | 20:58:07.67 +38:34:19.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.5319+38.5720,2461125.9688,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5319+38.5720 20260326.4688 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:58:04.10 +38:34:01.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.43 20:41:14.97 +34:27:38.2
75.70606 -4.60502 galactic Cyg Second-epoch detections are separated by 1.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1864136001142504704 | 20:41:14.90 +34:26:51.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1932MeUpp..55....1S BD+33 3990
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1864136001142504704,2461125.9688,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1864136001142504704 20260326.4688 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:41:14.97 +34:27:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4688 2461125.9688 14.46 20:13:43.09 +35:12:50.1
73.03057 0.42727 galactic Cyg Second-epoch detections are separated by 2.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.4168+35.2216 | 20:13:43.09 +35:12:50.1 (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 J303.4168+35.2216,2461125.9688,14.46,0.05,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 J303.4168+35.2216 20260326.4688 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-14-28_20.00sec_-14.90C_LIGHT_0685.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-06-Q2b1x1_061634_TTUQ2b1x1_28711_KmTBCLTq/fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20.00sec_-15.00C_LIGHT_0686.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:43.09 +35:12:50.1 ;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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_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_2026-03-26_06-15-13_20_00sec_-15_00C_LIGHT_0686_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_2026-03-26_06-14-28_20_00sec_-14_90C_LIGHT_0685_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.46 20:05:33.89 +29:30:38.3
67.30986 -1.23517 galactic Cyg Second-epoch detections are separated by 8.9" 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 2029359476010039808 | 20:05:33.33 +29:31:06.7 (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 2029359476010039808,2461125.9700,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2029359476010039808 20260326.4700 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:05:33.89 +29:30:38.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.29 19:57:01.57 +31:36:44.9
68.12316 1.43582 galactic Cyg Second-epoch detections are separated by 4.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.2580+31.6075 | 19:57:01.57 +31:36:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.2580+31.6075,2461125.9700,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2580+31.6075 20260326.4700 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:01.57 +31:36:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_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,2461125.9700,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4700 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:21:45.75 +31:48:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.37 20:16:17.00 +25:37:38.4
65.34449 -5.34248 galactic Vul Second-epoch detections are separated by 1.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.0730+25.6269 | 20:16:17.00 +25:37:38.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.0730+25.6269,2461125.9700,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.0730+25.6269 20260326.4700 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:17.00 +25:37:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 13.96 20:17:19.85 +32:51:46.0
71.49356 -1.50297 galactic Cyg Second-epoch detections are separated by 8.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2054572205341107968 | 20:17:19.63 +32:51:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2054572205341107968,2461125.9700,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2054572205341107968 20260326.4700 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:17:19.85 +32:51:46.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 13.09 19:51:11.46 +28:37:08.9
64.90693 0.97520 galactic Vul Second-epoch detections are separated by 4.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.7913+28.6106 | 19:51:10.61 +28:37:03.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.7913+28.6106,2461125.9700,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.7913+28.6106 20260326.4700 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:51:11.46 +28:37:08.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.24 20:24:37.22 +29:54:05.0
69.93203 -4.46234 galactic Cyg Second-epoch detections are separated by 5.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1861296478003973376 | 20:24:35.85 +29:54:46.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.923+/-0.040 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1861296478003973376,2461125.9700,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1861296478003973376 20260326.4700 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:37.22 +29:54:05.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.37 20:23:59.60 +31:51:44.6
71.46606 -3.22903 galactic Cyg Second-epoch detections are separated by 2.9" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.0066+31.8727 | 20:23:59.60 +31:51:44.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.689+/-0.155 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J306.0066+31.8727,2461125.9700,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J306.0066+31.8727 20260326.4700 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:59.60 +31:51:44.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_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,2461125.9700,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4700 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:51:15.12 +27:54:12.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_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,2461125.9700,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4700 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:39.75 +29:01:10.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.30 20:23:45.76 +32:14:22.6
71.74771 -2.97293 galactic Cyg Second-epoch detections are separated by 5.3" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.9364+32.2284 | 20:23:45.76 +32:14:22.6 (user input) | IRR (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 J305.9364+32.2284,2461125.9700,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J305.9364+32.2284 20260326.4700 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:45.76 +32:14:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.42 20:25:10.00 +28:59:51.2
69.25678 -5.07735 galactic Vul Second-epoch detections are separated by 8.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J202508.63+285922.8 | 20:25:08.63 +28:59:22.7 (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 J202508.63+285922.8,2461125.9700,14.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202508.63+285922.8 20260326.4700 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:10.00 +28:59:51.2 ;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_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.54 20:24:40.21 +31:44:48.5
71.45381 -3.41312 galactic Cyg Second-epoch detections are separated by 3.8" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.1684+31.7542 | 20:24:40.21 +31:44:48.5 (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 J306.1684+31.7542,2461125.9700,14.54,0.05,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
ATO J306.1684+31.7542 20260326.4700 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/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:40.21 +31:44:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_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,2461125.9700,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4700 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:46.05 +30:40:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.29 19:44:39.44 +28:27:41.3
64.04654 2.13457 galactic Cyg Second-epoch detections are separated by 8.0" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.1658+28.4508 | 19:44:37.65 +28:27:17.7 (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 J296.1658+28.4508,2461125.9700,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.1658+28.4508 20260326.4700 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:39.44 +28:27:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_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,2461125.9700,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4700 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:59.60 +30:42:43.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4700 2461125.9700 14.29 19:40:30.19 +28:43:11.1
63.81918 3.05472 galactic Cyg Second-epoch detections are separated by 5.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.1255+28.7292 | 19:40:30.19 +28:43:11.1 (user input) | CBF (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 J295.1255+28.7292,2461125.9700,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.1255+28.7292 20260326.4700 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-02-27_05-48-52_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20.00sec_-15.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-08-Q2b1x1_061833_TTUQ2b1x1_19331_ZReCwwOy/fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20.00sec_-14.90C_LIGHT_0688.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:30.19 +28:43:11.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-17-02_20_00sec_-14_90C_LIGHT_0688_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-08-Q2b1x1_2026-02-27_05-48-52_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png resample_wcs_fd_Cyg-08-Q2b1x1_2026-03-26_06-16-15_20_00sec_-15_00C_LIGHT_0687_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 26.4798* 18 44 13.15 +13 27 29.5 14.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9798,14.54,0.05,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 20260326.4798 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:44:13.15 +13:27:29.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.46 19:02:18.46 +16:56:12.9
49.26110 5.30584 galactic Aql Second-epoch detections are separated by 1.0" and 0.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J285.5766+16.9386 | 19:02:18.46 +16:56:12.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J285.5766+16.9386,2461125.9798,14.46,0.05,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 J285.5766+16.9386 20260326.4798 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:02:18.46 +16:56:12.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.50 18:59:16.57 +13:18:54.1
45.68618 4.32427 galactic Aql 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 | ATO J284.8162+13.3160 | 18:59:16.57 +13:18:54.1 (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 J284.8162+13.3160,2461125.9798,14.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J284.8162+13.3160 20260326.4798 14.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:59:16.57 +13:18:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.19 18:18:41.20 +11:23:56.6
39.53036 12.37867 galactic Oph Second-epoch detections are separated by 1.7" 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 4484508154142408320 | 18:18:39.50 +11:23:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4484508154142408320,2461125.9798,14.19,0.05,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 4484508154142408320 20260326.4798 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:18:41.20 +11:23:56.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.24 18:53:14.27 +10:51:31.2
42.81954 4.53322 galactic Aql Second-epoch detections are separated by 3.6" 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 | ATO J283.3154+10.8528 | 18:53:14.27 +10:51:31.2 (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 J283.3154+10.8528,2461125.9798,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.3154+10.8528 20260326.4798 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:53:14.27 +10:51:31.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 13.99 18:51:24.13 +11:06:08.5
42.83457 5.04520 galactic Aql Second-epoch detections are separated by 3.4" 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 | Gaia DR3 4504174951160442112 | 18:51:25.28 +11:06:09.7 (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 4504174951160442112,2461125.9798,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4504174951160442112 20260326.4798 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:51:24.13 +11:06:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 13.95 18:44:25.18 +12:34:04.7
43.38758 7.22799 galactic Her Second-epoch detections are separated by 2.2" 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 | ASASSN-V J184427.09+123332.6 | 18:44:27.09 +12:33:32.6 (Gaia DR3) | SR (local) | 2458671.98500 (local) | Gaia3var=VARIABLE J-Ks=0.623+/-0.049 (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 26.4798* 18 44 25.18 +12 34 04.7 13.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J184427.09+123332.6,2461125.9798,13.95,0.05,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
ASASSN-V J184427.09+123332.6 20260326.4798 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:44:25.18 +12:34:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.38 19:01:18.81 +16:40:36.0
48.92012 5.40115 galactic Aql Second-epoch detections are separated by 0.4" and 0.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J285.3227+16.6691 | 19:01:18.81 +16:40:36.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J285.3227+16.6691,2461125.9798,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J285.3227+16.6691 20260326.4798 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:01:18.81 +16:40:36.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.35 19:00:47.03 +12:22:39.5
45.01540 3.57198 galactic Aql Second-epoch detections are separated by 4.0" 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 | Gaia DR3 4313768807396028288 | 19:00:48.49 +12:22:35.2 (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 4313768807396028288,2461125.9798,14.35,0.05,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
Gaia DR3 4313768807396028288 20260326.4798 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:00:47.03 +12:22:39.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.31 18:56:12.59 +14:06:43.0
46.06363 5.34810 galactic Her Second-epoch detections are separated by 4.6" 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 | ASASSN-V J185611.12+140707.2 | 18:56:11.12 +14:07:07.1 (Gaia DR3) | SR (local) | 102.000000000000 (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 26.4798* 18 56 12.59 +14 06 43.0 14.3 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
ASASSN-V J185611.12+140707.2,2461125.9798,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185611.12+140707.2 20260326.4798 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:56:12.59 +14:06:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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 26.4798* 18 50 23.72 +12 29 38.5 14.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9798,14.46,0.05,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 20260326.4798 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:50:23.72 +12:29:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.44 18:56:32.30 +12:30:17.8
44.65908 4.55387 galactic Her Second-epoch detections are separated by 5.5" 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 | Large-amplitude variable Gaia DR2 4505881771132843008 | 18:56:34.71 +12:30:44.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.4798* 18 56 32.30 +12 30 17.8 14.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 4505881771132843008,2461125.9798,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4505881771132843008 20260326.4798 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:56:32.30 +12:30:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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 26.4798* 18 51 08.38 +17 51 14.2 14.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9798,14.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4798 14.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:51:08.38 +17:51:14.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.56 18:59:06.71 +17:06:03.2
49.06382 6.06214 galactic Aql Second-epoch detections are separated by 2.7" 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 | ATO J284.7764+17.1015 | 18:59:06.71 +17:06:03.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.799+/-0.049 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J284.7764+17.1015,2461125.9798,14.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J284.7764+17.1015 20260326.4798 14.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:59:06.71 +17:06:03.2 ;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_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4798 2461125.9798 14.70 18:58:48.78 +16:55:21.3
48.87132 6.04633 galactic Aql Second-epoch detections are separated by 3.2" 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 | ATO J284.6952+16.9255 | 18:58:48.78 +16:55:21.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J284.6952+16.9255,2461125.9798,14.70,0.05,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 J284.6952+16.9255 20260326.4798 14.70CV 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/Her-10-Q2b1x1_2026-02-27_05-54-33_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-30-26_20.00sec_-14.90C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-10-Q2b1x1_063237_TTUQ2b1x1_26038_3U7UJV7X/fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:58:48.78 +16:55:21.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-10-Q2b1x1_2026-02-27_05-54-33_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Her-10-Q2b1x1_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_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_2026-03-26_06-31-11_20_00sec_-15_00C_LIGHT_0704_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_2026-03-26_06-30-26_20_00sec_-14_90C_LIGHT_0703_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.44 19:04:00.85 +23:49:04.2
55.64131 8.01800 galactic Vul Second-epoch detections are separated by 6.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J285.9988+23.8195 | 19:04:00.85 +23:49:04.2 (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 J285.9988+23.8195,2461125.9761,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J285.9988+23.8195 20260326.4761 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:04:00.85 +23:49:04.2 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_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,2461125.9761,14.18,0.05,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 20260326.4761 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:01:47.85 +25:34:31.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.28 18:54:22.65 +18:16:44.3
49.62308 7.59545 galactic Her Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J283.5943+18.2773 | 18:54:22.65 +18:16:44.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.4761* 18 54 22.65 +18 16 44.3 14.3 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 J283.5943+18.2773,2461125.9761,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.5943+18.2773 20260326.4761 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:54:22.65 +18:16:44.3 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.31 19:42:28.56 +24:15:21.6
60.15477 0.46497 galactic Vul Second-epoch detections are separated by 3.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.6259+24.2559 | 19:42:27.97 +24:15:37.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.867+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.6259+24.2559,2461125.9761,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.6259+24.2559 20260326.4761 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:28.56 +24:15:21.6 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.18 19:23:59.96 +25:52:41.9
59.55913 4.91256 galactic Vul Second-epoch detections are separated by 3.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.0117+25.8804 | 19:23:59.96 +25:52:41.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.451+/-0.047 (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 J291.0117+25.8804,2461125.9761,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J291.0117+25.8804 20260326.4761 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:23:59.96 +25:52:41.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.12 19:38:40.05 +25:40:43.0
60.96653 1.91760 galactic Vul Second-epoch detections are separated by 6.8" 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 2021861803185528576 | 19:38:39.73 +25:41:01.2 (Gaia DR3) | (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
Gaia DR3 2021861803185528576,2461125.9761,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2021861803185528576 20260326.4761 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:38:40.05 +25:40:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 13.94 18:55:18.91 +19:04:50.8
50.44817 7.74896 galactic Her Second-epoch detections are separated by 6.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J283.8265+19.0780 | 18:55:18.91 +19:04:50.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.4761* 18 55 18.91 +19 04 50.8 13.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J283.8265+19.0780,2461125.9761,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.8265+19.0780 20260326.4761 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/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:55:18.91 +19:04:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.33 19:43:36.64 +25:53:10.6
61.69710 1.05273 galactic Vul Second-epoch detections are separated by 5.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2021775658964927232 | 19:43:35.82 +25:53:42.3 (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 2021775658964927232,2461125.9761,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2021775658964927232 20260326.4761 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:36.64 +25:53:10.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.27 19:23:03.25 +22:18:35.8
56.29625 3.43258 galactic Vul Second-epoch detections are separated by 4.4" 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 J290.7484+22.3111 | 19:23:00.78 +22:18:26.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J290.7484+22.3111,2461125.9761,14.27,0.05,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
ATO J290.7484+22.3111 20260326.4761 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/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:23:03.25 +22:18:35.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.14 19:03:46.67 +18:18:14.9
50.64588 5.60868 galactic Aql Second-epoch detections are separated by 2.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J285.9432+18.3020 | 19:03:46.67 +18:18:14.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.734+/-0.179 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J285.9432+18.3020,2461125.9761,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J285.9432+18.3020 20260326.4761 14.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:03:46.67 +18:18:14.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.35 19:33:34.59 +23:14:58.8
58.27954 1.74730 galactic Vul Second-epoch detections are separated by 0.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2019495890324876544 | 19:33:33.89 +23:14:32.2 (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 2019495890324876544,2461125.9761,14.35,0.05,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
Gaia DR3 2019495890324876544 20260326.4761 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/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:34.59 +23:14:58.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.54 19:44:52.10 +22:47:41.8
59.16130 -0.73854 galactic Vul Second-epoch detections are separated by 1.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.2156+22.8018 | 19:44:52.10 +22:47:41.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.2156+22.8018,2461125.9761,14.54,0.05,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
ATO J296.2156+22.8018 20260326.4761 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/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:52.10 +22:47:41.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 14.44 18:57:35.13 +18:18:19.9
49.98640 6.92414 galactic Aql Second-epoch detections are separated by 6.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4517349265116655744 | 18:57:33.05 +18:18:02.7 (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 4517349265116655744,2461125.9761,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4517349265116655744 20260326.4761 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:57:35.13 +18:18:19.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4761 2461125.9761 13.12 19:43:48.29 +24:46:27.0
60.75465 0.46055 galactic Vul Second-epoch detections are separated by 0.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.9544+24.7773 | 19:43:48.62 +24:46:22.7 (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 J295.9544+24.7773,2461125.9761,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.9544+24.7773 20260326.4761 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20.00sec_-14.90C_LIGHT_0697.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vul-01-Q2b1x1_062636_TTUQ2b1x1_16834_G9MDWint/fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20.00sec_-14.90C_LIGHT_0698.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:48.29 +24:46:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-53_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-26_06-25-01_20_00sec_-14_90C_LIGHT_0697_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 14.30 21:20:38.32 +45:40:30.0
89.11564 -2.90245 galactic Cyg Second-epoch detections are separated by 2.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.1439+45.6819 | 21:20:38.32 +45:40:30.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J320.1439+45.6819,2461125.9736,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J320.1439+45.6819 20260326.4736 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:20:38.32 +45:40:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 14.26 22:00:12.58 +48:18:47.2
95.93601 -5.37749 galactic Cyg Second-epoch detections are separated by 1.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.0503+48.3109 | 22:00:12.58 +48:18:47.2 (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 J330.0503+48.3109,2461125.9736,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.0503+48.3109 20260326.4736 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:00:12.58 +48:18:47.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 14.02 21:01:54.71 +44:29:54.9
85.99585 -1.29435 galactic Cyg Second-epoch detections are separated by 8.7" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4830+44.4993 | 21:01:57.70 +44:30:07.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4830+44.4993,2461125.9736,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4830+44.4993 20260326.4736 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:01:54.71 +44:29:54.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 13.99 21:56:53.71 +47:30:51.0
95.00339 -5.66906 galactic Cyg Second-epoch detections are separated by 2.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.2373+47.5063 | 21:56:54.96 +47:30:14.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.2373+47.5063,2461125.9736,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.2373+47.5063 20260326.4736 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:56:53.71 +47:30:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 13.71 21:26:41.86 +46:27:26.6
90.41515 -3.08254 galactic Cyg Second-epoch detections are separated by 2.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.6766+46.4588 | 21:26:39.90 +46:27:16.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.6766+46.4588,2461125.9736,13.71,0.05,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
ATO J321.6766+46.4588 20260326.4736 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/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:41.86 +46:27:26.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 13.59 21:26:06.42 +46:08:36.8
90.12319 -3.23719 galactic Cyg Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1972083991171005056 | 21:26:06.15 +46:08:45.7 (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 1972083991171005056,2461125.9736,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972083991171005056 20260326.4736 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:06.42 +46:08:36.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 13.96 21:49:44.00 +48:49:08.4
94.88930 -3.90402 galactic Cyg 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 J327.4345+48.8164 | 21:49:44.00 +48:49:08.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.516+/-0.170 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J327.4345+48.8164,2461125.9736,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.4345+48.8164 20260326.4736 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:44.00 +48:49:08.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 13.97 21:43:28.75 +46:14:48.9
92.41677 -5.19026 galactic Cyg Second-epoch detections are separated by 1.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | V0653 Cyg | 21:43:28.45 +46:15:20.7 (Gaia DR3) | SRA (local) | 312.000000000000 (local) | Gaia3var=VARIABLE SpType: M6.5 1956ApJ...124..346C V653 Cyg
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0653 Cyg,2461125.9736,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0653 Cyg 20260326.4736 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:28.75 +46:14:48.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 14.18 21:57:46.15 +47:31:55.9
95.13136 -5.74574 galactic Cyg Second-epoch detections are separated by 2.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J329.4402+47.5197 | 21:57:42.52 +47:31:45.0 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.4402+47.5197,2461125.9736,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.4402+47.5197 20260326.4736 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:46.15 +47:31:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 14.21 21:23:37.23 +45:22:16.4
89.27168 -3.48622 galactic Cyg Second-epoch detections are separated by 3.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.9078+45.3742 | 21:23:37.23 +45:22:16.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J320.9078+45.3742,2461125.9736,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J320.9078+45.3742 20260326.4736 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:23:37.23 +45:22:16.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 14.24 21:34:19.19 +44:07:51.9
89.79235 -5.69443 galactic Cyg Second-epoch detections are separated by 4.0" 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 | V0629 Cyg | 21:34:15.22 +44:07:57.8 (Gaia DR3) | LB (local) | (local) | Gaia3var=VARIABLE SpType: M4 1947AnDea...5....1L DO 39770
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0629 Cyg,2461125.9736,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0629 Cyg 20260326.4736 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:19.19 +44:07:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 14.33 21:34:22.91 +48:42:55.8
92.90828 -2.32423 galactic Cyg Second-epoch detections are separated by 2.7" 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 J323.5961+48.7177 | 21:34:22.91 +48:42:55.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J323.5961+48.7177,2461125.9736,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J323.5961+48.7177 20260326.4736 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:34:22.91 +48:42:55.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4736 2461125.9736 14.38 21:49:33.87 +47:06:15.1
93.77292 -5.20900 galactic Cyg Second-epoch detections are separated by 1.8" 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 | ATO J327.4035+47.1130 | 21:49:33.87 +47:06:15.1 (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 J327.4035+47.1130,2461125.9736,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.4035+47.1130 20260326.4736 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:33.87 +47:06:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_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,2461125.9736,14.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4736 14.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:15.70 +44:07:33.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_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
V0613 Cyg,2461125.9736,14.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0613 Cyg 20260326.4736 14.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-26_19-21-11_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20.00sec_-14.90C_LIGHT_0693.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cyg-04-Q2b1x1_062439_TTUQ2b1x1_15984_LktM84vq/fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20.00sec_-14.90C_LIGHT_0694.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:30.22 +42:57:33.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-22-17_20_00sec_-14_90C_LIGHT_0694_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-26_19-21-11_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-03-26_06-21-29_20_00sec_-14_90C_LIGHT_0693_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 14.45 19:35:54.32 +12:57:26.6
49.54115 -3.72606 galactic Aql Second-epoch detections are separated by 1.0" 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 J293.9778+12.9617 | 19:35:54.32 +12:57:26.6 (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 J293.9778+12.9617,2461125.9809,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.9778+12.9617 20260326.4809 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:35:54.32 +12:57:26.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 14.46 19:45:28.93 +12:24:10.4
50.20028 -6.03521 galactic Aql Second-epoch detections are separated by 3.2" 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 | ASASSN-V J194530.97+122350.8 | 19:45:30.97 +12:23:50.8 (Gaia DR3) | SR (local) | 2458311.59100 (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 J194530.97+122350.8,2461125.9809,14.46,0.05,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
ASASSN-V J194530.97+122350.8 20260326.4809 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:28.93 +12:24:10.4 ;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-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 14.18 19:19:07.85 +14:39:26.7
49.09639 0.66433 galactic Aql Second-epoch detections are separated by 3.2" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:19:07.85 +14:39:26.7 (user input) | T | P | (position from user input) J-Ks=1.704+/-0.053 (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,2461125.9809,14.18,0.05,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 20260326.4809 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:19:07.85 +14:39:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 13.93 19:41:24.78 +13:18:08.3
50.49778 -4.72950 galactic Aql Second-epoch detections are separated by 3.1" 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 | ATO J295.3526+13.3040 | 19:41:24.78 +13:18:08.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.3526+13.3040,2461125.9809,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.3526+13.3040 20260326.4809 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/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:24.78 +13:18:08.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 13.95 19:49:03.55 +14:26:38.8
52.41588 -5.77798 galactic Aql Second-epoch detections are separated by 3.9" 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 | ASAS J194902+1426.3 | 19:49:02.41 +14:26:15.1 (Gaia DR3) | MISC (local) | 2452831.30000 (local) | Gaia3var=VARIABLE SpType: M3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J194902+1426.3,2461125.9809,13.95,0.05,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
ASAS J194902+1426.3 20260326.4809 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/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:03.55 +14:26:38.8 ;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_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 14.24 19:47:23.89 +15:59:33.3
53.56218 -4.65761 galactic Aql Second-epoch detections are separated by 1.7" 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 J296.8502+16.0041 | 19:47:23.89 +15:59:33.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.8502+16.0041,2461125.9809,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.8502+16.0041 20260326.4809 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:47:23.89 +15:59:33.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 14.03 19:44:33.47 +17:48:17.5
54.79762 -3.16537 galactic Sge Second-epoch detections are separated by 3.9" 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 | ATO J296.1280+17.8078 | 19:44:33.47 +17:48:17.5 (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 J296.1280+17.8078,2461125.9809,14.03,0.05,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
ATO J296.1280+17.8078 20260326.4809 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/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:33.47 +17:48:17.5 ;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_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 14.10 19:51:58.42 +16:57:58.6
54.96032 -5.11654 galactic Sge Second-epoch detections are separated by 1.6" 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 J298.0054+16.9632 | 19:51:58.42 +16:57:58.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.826+/- (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.0054+16.9632,2461125.9809,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.0054+16.9632 20260326.4809 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:51:58.42 +16:57:58.6 ;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-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 14.29 19:53:32.76 +16:31:16.7
54.76656 -5.66652 galactic Sge Second-epoch detections are separated by 0.9" 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 J298.3867+16.5120 | 19:53:32.76 +16:31:16.7 (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 J298.3867+16.5120,2461125.9809,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.3867+16.5120 20260326.4809 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:53:32.76 +16:31:16.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 14.36 19:47:12.75 +17:49:50.2
55.13589 -3.70003 galactic Sge Second-epoch detections are separated by 4.8" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.8045+17.8361 | 19:47:12.75 +17:49:50.2 (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 J296.8045+17.8361,2461125.9809,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.8045+17.8361 20260326.4809 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:47:12.75 +17:49:50.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4809 2461125.9809 14.41 19:56:53.18 +17:10:24.6
55.74020 -6.02146 galactic Sge Second-epoch detections are separated by 2.4" 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 | ATO J299.2206+17.1760 | 19:56:53.18 +17:10:24.6 (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 J299.2206+17.1760,2461125.9809,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2206+17.1760 20260326.4809 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q2b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20.00sec_-15.00C_LIGHT_0705.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-01-Q2b1x1_063433_TTUQ2b1x1_21602_LqR1hNU9/fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20.00sec_-15.00C_LIGHT_0706.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:56:53.18 +17:10:24.6 ;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-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-32-43_20_00sec_-15_00C_LIGHT_0706_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-01-Q2b1x1_2026-02-27_05-56-11_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png resample_wcs_fd_Aql-01-Q2b1x1_2026-03-26_06-31-59_20_00sec_-15_00C_LIGHT_0705_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4869 2461125.9869 14.19 21:24:10.76 +63:49:57.1
102.35016 9.59104 galactic Cep Second-epoch detections are separated by 3.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:24:10.76 +63:49:57.1 (user input) | T | P | (position from user input) J-Ks=0.488+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9869,14.19,0.05,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 20260326.4869 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-26_19-31-09_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_064437_TTUQ2b1x1_26251_V9gXrJFF/fd_Cep-06-Q2b1x1_2026-03-26_06-40-31_20.00sec_-14.90C_LIGHT_0715.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_064437_TTUQ2b1x1_26251_V9gXrJFF/fd_Cep-06-Q2b1x1_2026-03-26_06-41-28_20.00sec_-15.00C_LIGHT_0716.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:24:10.76 +63:49:57.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-41-28_20_00sec_-15_00C_LIGHT_0716_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-40-31_20_00sec_-14_90C_LIGHT_0715_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-41-28_20_00sec_-15_00C_LIGHT_0716_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-40-31_20_00sec_-14_90C_LIGHT_0715_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4869 2461125.9869 13.90 21:44:22.18 +63:17:31.1
103.63859 7.66309 galactic Cep Second-epoch detections are separated by 6.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2216648018930963968 | 21:44:15.35 +63:17:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2216648018930963968,2461125.9869,13.90,0.05,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 2216648018930963968 20260326.4869 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/Cep-06-Q2b1x1_2025-12-26_19-31-09_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_064437_TTUQ2b1x1_26251_V9gXrJFF/fd_Cep-06-Q2b1x1_2026-03-26_06-40-31_20.00sec_-14.90C_LIGHT_0715.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_064437_TTUQ2b1x1_26251_V9gXrJFF/fd_Cep-06-Q2b1x1_2026-03-26_06-41-28_20.00sec_-15.00C_LIGHT_0716.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:44:22.18 +63:17:31.1 ;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_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-41-28_20_00sec_-15_00C_LIGHT_0716_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-40-31_20_00sec_-14_90C_LIGHT_0715_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-41-28_20_00sec_-15_00C_LIGHT_0716_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-40-31_20_00sec_-14_90C_LIGHT_0715_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,2461125.9869,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4869 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-26_19-31-09_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_064437_TTUQ2b1x1_26251_V9gXrJFF/fd_Cep-06-Q2b1x1_2026-03-26_06-40-31_20.00sec_-14.90C_LIGHT_0715.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cep-06-Q2b1x1_064437_TTUQ2b1x1_26251_V9gXrJFF/fd_Cep-06-Q2b1x1_2026-03-26_06-41-28_20.00sec_-15.00C_LIGHT_0716.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:56.41 +58:58:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-41-28_20_00sec_-15_00C_LIGHT_0716_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-40-31_20_00sec_-14_90C_LIGHT_0715_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-41-28_20_00sec_-15_00C_LIGHT_0716_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-26_19-31-09_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-26_06-40-31_20_00sec_-14_90C_LIGHT_0715_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4856 2461125.9856 11.52 18:50:55.04 -06:17:31.1
27.26867 -2.74920 galactic Sct Second-epoch detections are separated by 6.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4252502443363639936 | 18:50:55.82 -06:18:14.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1922ApJ....55...85L NGC 6705 Str 237
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4252502443363639936,2461125.9856,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4252502443363639936 20260326.4856 11.52CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20.00sec_-15.00C_LIGHT_0713.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20.00sec_-15.00C_LIGHT_0714.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:50:55.04 -06:17:31.1 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4856 2461125.9856 13.90 19:13:46.84 +01:15:27.2
36.60668 -4.39305 galactic Aql Second-epoch detections are separated by 0.3" 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 J288.4468+01.2588 | 19:13:47.98 +01:14:52.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J288.4468+01.2588,2461125.9856,13.90,0.05,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
ATO J288.4468+01.2588 20260326.4856 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20.00sec_-15.00C_LIGHT_0713.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20.00sec_-15.00C_LIGHT_0714.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:13:46.84 +01:15:27.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4856 2461125.9856 14.23 19:11:57.68 +00:53:15.1
36.06777 -4.15872 galactic Aql Second-epoch detections are separated by 4.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.9802+00.8929 | 19:11:57.68 +00:53:15.1 (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 J287.9802+00.8929,2461125.9856,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.9802+00.8929 20260326.4856 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20.00sec_-15.00C_LIGHT_0713.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20.00sec_-15.00C_LIGHT_0714.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:11:57.68 +00:53:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4856 2461125.9856 14.16 18:59:12.44 -05:24:27.3
28.99435 -4.18648 galactic Aql Second-epoch detections are separated by 2.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J284.8098-05.4124 | 18:59:12.44 -05:24:27.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.518+/-0.082 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J284.8098-05.4124,2461125.9856,14.16,0.05,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 J284.8098-05.4124 20260326.4856 14.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20.00sec_-15.00C_LIGHT_0713.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20.00sec_-15.00C_LIGHT_0714.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:59:12.44 -05:24:27.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4856 2461125.9856 14.38 19:02:08.14 -04:53:14.7
29.79038 -4.60153 galactic Aql Second-epoch detections are separated by 6.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J285.5372-04.8826 | 19:02:08.14 -04:53:14.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=2.700+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J285.5372-04.8826,2461125.9856,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J285.5372-04.8826 20260326.4856 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20.00sec_-15.00C_LIGHT_0713.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-03-Q2b1x1_064235_TTUQ2b1x1_20578_W9wH8Tz9/fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20.00sec_-15.00C_LIGHT_0714.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:02:08.14 -04:53:14.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-39-34_20_00sec_-15_00C_LIGHT_0714_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-26_06-38-43_20_00sec_-15_00C_LIGHT_0713_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 26.4881* 23 58 59.89 +54 43 26.1 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9881,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4881 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-04-Q2b1x1_064637_TTUQ2b1x1_19042_GSb76bh1/fd_Cas-04-Q2b1x1_2026-03-26_06-42-17_20.00sec_-14.90C_LIGHT_0717.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Cas-04-Q2b1x1_064637_TTUQ2b1x1_19042_GSb76bh1/fd_Cas-04-Q2b1x1_2026-03-26_06-43-08_20.00sec_-14.90C_LIGHT_0718.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:58:59.89 +54:43:26.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-04-Q2b1x1_2025-12-26_19-59-31_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png resample_wcs_fd_Cas-04-Q2b1x1_2026-03-26_06-43-08_20_00sec_-14_90C_LIGHT_0718_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q2b1x1_2025-12-26_19-59-31_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png resample_wcs_fd_Cas-04-Q2b1x1_2026-03-26_06-42-17_20_00sec_-14_90C_LIGHT_0717_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-26_19-59-31_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png resample_wcs_fd_Cas-04-Q2b1x1_2026-03-26_06-43-08_20_00sec_-14_90C_LIGHT_0718_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q2b1x1_2025-12-26_19-59-31_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png resample_wcs_fd_Cas-04-Q2b1x1_2026-03-26_06-42-17_20_00sec_-14_90C_LIGHT_0717_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,2461125.9831,14.16,0.05,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
target 20260326.4831 14.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:26.53 +09:50:26.0 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4831 2461125.9831 13.83 19:26:41.66 +05:07:06.0
41.53966 -5.45987 galactic Aql Second-epoch detections are separated by 3.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.6756+05.1163 | 19:26:41.66 +05:07:06.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J291.6756+05.1163,2461125.9831,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J291.6756+05.1163 20260326.4831 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:26:41.66 +05:07:06.0 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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,2461125.9831,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.4831 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:23:44.96 +09:29:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4831 2461125.9831 13.64 19:33:32.59 +08:27:46.7
45.30744 -5.37717 galactic Aql Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4296072103366193792 | 19:33:33.12 +08:27:50.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4296072103366193792,2461125.9831,13.64,0.05,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
Gaia DR3 4296072103366193792 20260326.4831 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:32.59 +08:27:46.7 ;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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4831 2461125.9831 13.43 19:33:10.77 +09:29:46.9
46.17594 -4.80478 galactic Aql Second-epoch detections are separated by 8.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4302375740965426816 | 19:33:09.05 +09:29:56.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4302375740965426816,2461125.9831,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4302375740965426816 20260326.4831 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:10.77 +09:29:46.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4831 2461125.9831 14.20 20:05:16.71 +08:19:01.9
49.07148 -12.29158 galactic Aql Second-epoch detections are separated by 7.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J301.3152+08.3150 | 20:05:16.71 +08:19:01.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.3152+08.3150,2461125.9831,14.20,0.05,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
ATO J301.3152+08.3150 20260326.4831 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:05:16.71 +08:19:01.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4831 2461125.9831 14.31 20:07:16.24 +06:35:43.9
47.79783 -13.58277 galactic Aql Second-epoch detections are separated by 2.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J301.8187+06.5992 | 20:07:16.24 +06:35:43.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.8187+06.5992,2461125.9831,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J301.8187+06.5992 20260326.4831 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:07:16.24 +06:35:43.9 ;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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4831 2461125.9831 14.27 19:49:41.83 +09:08:44.8
47.85526 -8.53927 galactic Aql Second-epoch detections are separated by 7.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4301648001685548672 | 19:49:40.93 +09:09:25.1 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4301648001685548672,2461125.9831,14.27,0.05,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
Gaia DR3 4301648001685548672 20260326.4831 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:41.83 +09:08:44.8 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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,2461125.9831,14.19,0.05,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 20260326.4831 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:55.05 +08:58:38.0 ;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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png resample_wcs_fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4831 2461125.9831 14.32 19:18:08.24 +04:43:24.6
40.19244 -3.75827 galactic Aql Second-epoch detections are separated by 3.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J289.5390+04.7232 | 19:18:08.24 +04:43:24.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.043+/-0.060 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J289.5390+04.7232,2461125.9831,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.5390+04.7232 20260326.4831 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-05_20.00sec_-14.90C_LIGHT_0709.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aql-02-Q2b1x1_063836_TTUQ2b1x1_13480_wVJkjAY9/fd_Aql-02-Q2b1x1_2026-03-26_06-35-58_20.00sec_-15.00C_LIGHT_0710.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:18:08.24 +04:43:24.6 ;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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_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_2026-03-26_06-35-58_20_00sec_-15_00C_LIGHT_0710_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_2026-03-26_06-35-05_20_00sec_-14_90C_LIGHT_0709_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 14.24 18:38:01.88 +06:19:40.5
37.05919 5.85280 galactic Ser Second-epoch detections are separated by 1.6" 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 J279.5097+06.3268 | 18:38:01.88 +06:19:40.5 (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!
TCP 2026 03 26.4820* 18 38 01.88 +06 19 40.5 14.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J279.5097+06.3268,2461125.9820,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J279.5097+06.3268 20260326.4820 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:38:01.88 +06:19:40.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 14.19 19:16:02.28 +10:05:19.6
44.70393 -0.80191 galactic Aql Second-epoch detections are separated by 1.2" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:16:02.28 +10:05:19.6 (user input) | T | P | (position from user input) J-Ks=2.439+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.9820,14.19,0.05,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 20260326.4820 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:16:02.28 +10:05:19.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 13.62 18:34:38.30 +09:03:04.8
39.13419 7.82240 galactic Oph Second-epoch detections are separated by 1.9" 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 J278.6685+09.0518 | 18:34:38.30 +09:03:04.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J278.6685+09.0518,2461125.9820,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J278.6685+09.0518 20260326.4820 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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:34:38.30 +09:03:04.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 13.79 19:06:24.38 +03:57:08.4
38.15680 -1.51955 galactic Aql Second-epoch detections are separated by 2.9" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4269342803910239488 | 19:06:24.50 +03:57:16.2 (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 4269342803910239488,2461125.9820,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4269342803910239488 20260326.4820 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:06:24.38 +03:57:08.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 13.32 18:29:05.46 +09:34:41.5
38.99943 9.28279 galactic Oph Second-epoch detections are separated by 5.6" 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 J277.2733+09.5773 | 18:29:05.46 +09:34:41.5 (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 J277.2733+09.5773,2461125.9820,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J277.2733+09.5773 20260326.4820 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:29:05.46 +09:34:41.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 14.09 18:49:01.78 +10:13:18.2
41.78180 5.17059 galactic Aql Second-epoch detections are separated by 2.6" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASAS J184859+1013.5 | 18:48:59.56 +10:13:28.5 (Gaia DR3) | MISC (local) | 2452505.70000 (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184859+1013.5,2461125.9820,14.09,0.05,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
ASAS J184859+1013.5 20260326.4820 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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:49:01.78 +10:13:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 14.22 19:14:47.94 +05:41:50.4
40.67072 -2.57039 galactic Aql Second-epoch detections are separated by 2.2" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J288.6845+05.6844 | 19:14:46.59 +05:41:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J288.6845+05.6844,2461125.9820,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.6845+05.6844 20260326.4820 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:14:47.94 +05:41:50.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 14.40 18:55:46.05 +10:06:33.5
42.43086 3.63994 galactic Aql Second-epoch detections are separated by 3.0" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J283.9338+10.1097 | 18:55:46.05 +10:06:33.5 (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 J283.9338+10.1097,2461125.9820,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.9338+10.1097 20260326.4820 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:55:46.05 +10:06:33.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 14.27 18:23:53.07 +08:10:09.7
37.14166 9.81414 galactic Oph Second-epoch detections are separated by 4.3" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4478479257010938368 | 18:23:51.47 +08:09:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4478479257010938368,2461125.9820,14.27,0.05,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
Gaia DR3 4478479257010938368 20260326.4820 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/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:23:53.07 +08:10:09.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4820 2461125.9820 14.41 18:34:58.22 +07:26:32.8
37.71870 7.03173 galactic Oph Second-epoch detections are separated by 1.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4478840996334928768 | 18:34:55.57 +07:26:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4478840996334928768,2461125.9820,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4478840996334928768 20260326.4820 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-04-Q2b1x1_2026-03-22_04-27-01_20.00sec_-14.90C_LIGHT_0267.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20.00sec_-15.00C_LIGHT_0707.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-04-Q2b1x1_063636_TTUQ2b1x1_12696_JOM2KAjW/fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20.00sec_-14.90C_LIGHT_0708.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:34:58.22 +07:26:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-34-16_20_00sec_-14_90C_LIGHT_0708_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-04-Q2b1x1_2026-03-22_04-27-01_20_00sec_-14_90C_LIGHT_0267_fits__*pix.png resample_wcs_fd_Ser-04-Q2b1x1_2026-03-26_06-33-31_20_00sec_-15_00C_LIGHT_0707_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4845 2461125.9845 12.98 17:39:38.69 -00:06:04.4
24.43725 15.86973 galactic Oph Second-epoch detections are separated by 0.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4372230188542007552 | 17:39:39.00 -00:06:43.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1958PMcCO..13b....V AG-00 2233
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4372230188542007552,2461125.9845,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4372230188542007552 20260326.4845 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-03-19_04-10-36_20.00sec_-15.00C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-07-Q2b1x1_064037_TTUQ2b1x1_14876_cp7sYsqa/fd_Ser-07-Q2b1x1_2026-03-26_06-37-03_20.00sec_-14.90C_LIGHT_0711.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-07-Q2b1x1_064037_TTUQ2b1x1_14876_cp7sYsqa/fd_Ser-07-Q2b1x1_2026-03-26_06-37-55_20.00sec_-15.00C_LIGHT_0712.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:39:38.69 -00:06:04.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-07-Q2b1x1_2026-03-19_04-10-36_20_00sec_-15_00C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Ser-07-Q2b1x1_2026-03-26_06-37-55_20_00sec_-15_00C_LIGHT_0712_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-07-Q2b1x1_2026-03-19_04-10-36_20_00sec_-15_00C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Ser-07-Q2b1x1_2026-03-26_06-37-03_20_00sec_-14_90C_LIGHT_0711_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-07-Q2b1x1_2026-03-19_04-10-36_20_00sec_-15_00C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Ser-07-Q2b1x1_2026-03-26_06-37-55_20_00sec_-15_00C_LIGHT_0712_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-07-Q2b1x1_2026-03-19_04-10-36_20_00sec_-15_00C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Ser-07-Q2b1x1_2026-03-26_06-37-03_20_00sec_-14_90C_LIGHT_0711_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4845 2461125.9845 14.28 18:13:51.00 -00:19:52.3
28.31943 8.20259 galactic Ser Second-epoch detections are separated by 2.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J273.4647-00.3402 | 18:13:53.26 -00:19:55.7 (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!
TCP 2026 03 26.4845* 18 13 51.00 +00 19 52.3 14.3 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.4647-00.3402,2461125.9845,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.4647-00.3402 20260326.4845 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ser-07-Q2b1x1_2026-03-19_04-10-36_20.00sec_-15.00C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-07-Q2b1x1_064037_TTUQ2b1x1_14876_cp7sYsqa/fd_Ser-07-Q2b1x1_2026-03-26_06-37-03_20.00sec_-14.90C_LIGHT_0711.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-07-Q2b1x1_064037_TTUQ2b1x1_14876_cp7sYsqa/fd_Ser-07-Q2b1x1_2026-03-26_06-37-55_20.00sec_-15.00C_LIGHT_0712.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:13:51.00 -00:19:52.3 ;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_Ser-07-Q2b1x1_2026-03-19_04-10-36_20_00sec_-15_00C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Ser-07-Q2b1x1_2026-03-26_06-37-55_20_00sec_-15_00C_LIGHT_0712_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-07-Q2b1x1_2026-03-19_04-10-36_20_00sec_-15_00C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Ser-07-Q2b1x1_2026-03-26_06-37-03_20_00sec_-14_90C_LIGHT_0711_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-07-Q2b1x1_2026-03-19_04-10-36_20_00sec_-15_00C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Ser-07-Q2b1x1_2026-03-26_06-37-55_20_00sec_-15_00C_LIGHT_0712_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-07-Q2b1x1_2026-03-19_04-10-36_20_00sec_-15_00C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Ser-07-Q2b1x1_2026-03-26_06-37-03_20_00sec_-14_90C_LIGHT_0711_fits__*pix.png animation_v2.gif