H. Muraishi

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

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

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

The CANGAROO-III project

cm

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

^{-2}

Present status of the 7-10 m telescope of CANGAROO II

s

TeV gamma ray emission from southern sky objects and CANGAROO project

^{-1}

Initial performance of CANGAROO-II 7m telescope

(

The SNR W28 at TeV energies

\ge 3.0\pm 0.9

Very High Energy Gamma-Ray Observations of PSR B1509–58 with the CANGAROO 3.8 Meter Telescope

TeV) and

Evidence for TeV gamma-ray emission from the shell type SNR RXJ1713.7-3946

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