Information and discussions about LAT common interests with the TeV community
Relevant VHE experiments
Name |
Type |
Ethresh |
|---|---|---|
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 |
50 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.
Experimental Issues
Optimizing variability studies
- Visibility tools
- * Unified VHE visibility tool
- * LAT visibility tool
- Alerts/transients/scheduled observations
- * VHE timetables
Analysis Issues
Spectral fitting tools
Collaboration & Policy Issues
Meetings
Friday Nov 4 2005: GLAST, GRB and TeV observations