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
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Creator :Masaki Mori
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