activity
20002009
most citedDetection of Sub-TeV Gamma-Rays from the Galactic Center Direction by CANGAROO-II

184 citations · 499 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2009★ 12 cited

Search for VHE gamma rays from SS433/W50 with the CANGAROO-II telescope

Sei. Hayashi, F. Kajino, T. Naito +48

SS433, located at the center of the supernova remnant W50, is a close proximity binary system consisting of a compact star and a normal star. Jets of material are directed outwards…

astro-ph2006★ 12 cited

Erratum: Detection of diffuse TeV gamma-ray emission from the nearby starburst galaxy NGC 253

C. Itoh, R. Enomoto, S. Yanagita +1

The CANGAROO-II telescope observed sub-TeV gamma-ray emission from the nearby starburst galaxy NGC 253. The emission region was extended with a radial size of 0.3-0.6 degree. On th…

astro-ph2006★ 38 cited

CANGAROO-III Observations of the supernova remnant RX J0852.04622

R. Enomoto, S. Watanabe, T. Tanimori et al

Sub-TeV gamma-ray emission from the North-West rim of the supernova remnant RX J0852.04622 was detected with the CANGAROO-II telescope and recently confirmed by the H.E.S.S. gro…

astro-ph2005★ 34 cited

A Search for sub-TeV Gamma-rays from the Vela Pulsar Region with CANGAROO-III

R. Enomoto, K. Tsuchiya, Y. Adachi +2

We made stereoscopic observations of the Vela Pulsar region with two of the 10 m diameter CANGAROO-III imaging atmospheric Cherenkov telescopes in January and February, 2004, in a…

astro-ph2005★ 73 cited

Detection of Gamma-rays around 1TeV from RX J0852.0-4622 by CANGAROO-II

H. Katagiri, R. Enomoto, L. T. Ksenofontov +1

We have detected gamma-ray emission at the 6sigma level at energies greater than 500GeV from the supernova remnant RX J0852.0-4622 (G266.2-1.2) using the CANGAROO-II Imaging Atmosp…

hep-ph2004★ 13 cited

Neutrino Oscillations in Intermediate States.II -- Wave Packets

A. Asahara, K. Ishikawa, T. Shimomura +1

We analyze oscillations of intermediate neutrinos in terms of the scattering of particles described by Gaussian wave packets. We study a scalar model as in a previous paper (I) but…