T. Konishi

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 Gamma Rays of up to 50 TeV from the Crab Nebula

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

Very High Energy Gamma Rays from the Vela Pulsar Direction

cm

TeV gamma ray emission from southern sky objects and CANGAROO project

^{-2}

TeV gamma-ray observations of southern BL Lacs with the CANGAROO 3.8-m imaging telescope

s

TeV gamma-ray observations of southern BL Lacs with the CANGAROO 3.8m Imaging Telescope

^{-1}

Very High Energy Gamma Rays from the Vela Pulsar/Nebula

(

TeV Gamma-ray Observations of Southern AGN with the CANGAROO 3.8m Telescople

\ge 3.0\pm 0.9

Observations of Pulsars, PSR 1509-58 and PSR 1259-63, by CANGAROO 3.8 m Telescope

TeV) and

Observation of Spectrum of TeV

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