A. Kawachi

DISCOVERY OF TEV GAMMA RAYS FROM SN1006: FURTHER EVIDENCE FOR THE SNR ORIGIN OF COSMIC RAYS

This paper reports the first discovery of TeV gamma-ray emission from a supernova remnant made with the CANGAROO 3.8 m Telescope. TeV gamma rays were detected at the sky position and extension coincident with the north-east (NE) rim of shell-type Supernova remnant (SNR) SN1006 (Type Ia). SN1006 has been a most likely candidate for an extended TeV Gamma-ray source, since the clear synchrotron X-ray emission from the rims was recently observed by ASCA (Koyama et al. 1995), which is a strong evidence of the existence of very high energy electrons up to hundreds of TeV in the SNR. The observed TeV gamma-ray flux was

Detection of Sub-TeV Gamma Rays from the Galactic Center Direction by CANGAROO-II

(2.4\pm 0.5(statistical) \pm 0.7(systematic)) \times 10^{-12}

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

cm

Design study of CANGAROO-III, stereoscopic imaging atmospheric Cherenkov telescopes for sub-TeV γ-ray detection

^{-2}

A Search for TeV Gamma-Ray Emission from the PSR B1259–63/SS 2883 Binary System with the CANGAROO-II 10 Meter Telescope

s

The Optical reflector system for the CANGAROO-II imaging atmospheric Cherenkov telescope

^{-1}

Cangaroo III observations of the supernova remnant RX J0852.0-4622

(

A Search for Sub-TeV Gamma Rays from the Vela Pulsar Region with CANGAROO-III

\ge 3.0\pm 0.9

CANGAROO III Search for Gamma Rays from Centaurus A and the ω Centauri Region

TeV) and

Development of an atmospheric Cherenkov imaging camera for the CANGAROO-III experiment

(4.6\pm 0.6 \pm 1.4) \times 10^{-12}