Information and discussions about LAT common interests with the TeV community
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Name | Type | Ethresh |
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Imaging Atmospheric Cherenkov | 120 GeV | |
Imaging Atmospheric Cherenkov | 120 GeV | |
CANGAROO | Imaging Atmospheric Cherenkov | 500 GeV |
MILAGRO | Air Shower | 400 GeV - 40 TeV (1) |
Imaging Atmospheric Cherenkov | <30 GeV |
(1) 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
- Visibility tools
- * Unified VHE visibility tool
- * LAT visibility tool
- Alerts/transients/scheduled observations
- * VHE timetables
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Spectral fitting tools
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Meetings
GLAST, GRB and TeV observations