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This page is meant to document the methods used in identifying Fermi sources as possible very high energy (VHE) / TeV candidates, as well as categorizing those sources that are good candidates (as determined by these methods) for VHE emission. This page will track observations, both successful and otherwise, and help determine ways of improving on these selection methods.

TeV Telescopes for observing Fermi VHE source candidates

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

MILAGRO

Air Shower

400 GeV - 40 TeV (2)

MAGIC

Imaging Atmospheric Cherenkov

50 GeV

We should verify the numbers in this table (ECF - 15 Sep 2009)

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