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Name | Type | Ethresh (1) |
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Imaging Atmospheric Cherenkov | 120 GeV | |
Imaging Atmospheric Cherenkov | 120 GeV | |
Imaging Atmospheric Cherenkov | 500 GeV | |
MILAGRO | Air Shower | 400 GeV - 40 TeV (2) |
Imaging Atmospheric Cherenkov | 50 GeV |
(1) We need to distinguish between anticipated threshold and achieved/documented threshold. Until then,
careful with these numbers be critical to the quoted number
(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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Optimizing variability studies
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Spectral fitting tools
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The object of desire: What we ought to know about the facilities
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