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titleRelevant VHE experiments
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Name

Type

Ethresh(1)

H.E.S.S.

Imaging Atmospheric Cherenkov

120 GeV

VERITAS-4

Imaging Atmospheric Cherenkov

120 GeV

CANGAROOIII

Imaging Atmospheric Cherenkov

500 GeV (question)

MILAGRO

Air Shower

400 GeV - 40 TeV (12)

MAGIC

Imaging Atmospheric Cherenkov

50 GeV (question)

(1) We need to distinguish between anticipated threshold and achieved/documented threshold. Until then,
careful with these numbers
(2) The threshold/energy response of a ground array like Milagro cannot easily be compared to ACTs. This interval respresents the energy range over which 90% of events from a crab-like spectrum are detected.

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