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Panel | ||||||||||
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| ||||||||||
Name | Type | Ethresh(1) |
---|---|---|
Imaging Atmospheric Cherenkov | 120 GeV | |
Imaging Atmospheric Cherenkov | 120 GeV | |
Imaging Atmospheric Cherenkov | 500 GeV | |
MILAGRO | Air Shower | 400 GeV - 40 TeV (12) |
Imaging Atmospheric Cherenkov | 50 GeV |
(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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