The CANGAROO-III Project

99/08/11


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Contents

The CANGAROO-III Project

CANGAROO Collaboration

CANGAROO Telescopes

New initiatives in ACTs

CANGAROO-III

10m telescope

Possible layout

CANGAROO-III Schedule

Expansion from 7m to 10m

Expected point image

Small spherical mirror

Mirror control

Mirror tuning

Camera

Electronics

Inter-telescope trigger

Simulation of stereo observation

Simulated Cherenkov image

Detection efficiency vs. separation

Angular/energy resolution

Single vs. stereo

Proton/gamma discrimination

Expected sensitivity

Sensitivity - XBLs

BL Lac Objects

Summary

Creator :Masaki Mori