Information and discussions about LAT common interests with the TeV community
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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, be critical to any 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
- Visibility tools proposals and tools H.E.S.S.
- * Unified VHE visibility tool
- * LAT visibility tool
- Alerts/transients/scheduled observations
- * VHE timetables
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Spectral fitting tools
VHE sources
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The object of desire: What we ought to know about the facilities
Facility | Object visibility/constraints | Analysis technique/data products | Comments |
template | energetic threshold = f(dec); low threshold cuts readily available ? | shower reconstruction: which MC/version ? |
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| point source sensitivity = f(dec); public? generally applicable ? | high-level data product: gamma-ray excess-map - availability / conditions ? |
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| extended source sensitivity = f(source size); public ? generally applicable ? | high-level data product: gamma-ray excess-map - format (root/fits) ? |
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| energy resolution public? known dependencies ? | high-level data product: spectral data - availability / conditions ? |
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| angular resolution public ? known dependencies ? | high-level data product: spectral data - format (xspect/root/...) ? |
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| timeline: observational history : which objectes ? when? eff. exposure? result published ? | high-level data product: spectral fits - fit-function flexibility ? which uncertainties ? |
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| schedules: which objects ? when ? result will be made available when ? | intent of matching contemporaneous analysis ? when ? how ? |
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| lc: minimal timescale ? flexibility in rebinning ? |
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Towards a Network of Atmospheric Cherenkov Detectors VII, April 2005, Paris
Meetings
Friday Nov 4 2005: GLAST, GRB and TeV observations
Saturday Mar 4 2006: F2F meeting
Wednesday, June 14, 2006 (9am Pacific): VRVS meeting in Vela