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Published byVera Dharmawijaya Modified over 6 years ago
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Mieke Bouwhuis on behalf of the ANTARES collaboration
Results from ANTARES Mieke Bouwhuis on behalf of the ANTARES collaboration TeV Particle Astrophysics 28-31 August 2006
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Data taking & data processing
Line 1 operational since March 2nd, 2006 Offline track reconstruction Physics events when enough correlated hits are found online data processing farm look for a muon-like signal using all registered hits DataFilter PC all data
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Line 1 Reconstruction uses first hit on a storey scan over directions
3-parameter fit, find all local minima for each local minimum, fit theta 4-parameter c2 fit best-fit selection, sort on c2 /dof
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Hit time residuals muon bundles scattered light line shape
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Display of a downgoing muon
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Downgoing muon
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Atmospheric muon bundles
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Cherenkov cone
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Showers
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Monte Carlo simulation of shower
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Multiple showers
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Zenith angle of atmospheric muons
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Upgoing muon candidate
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Event times
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Conclusions Line 1 operational First results
Ambiguity suppressed using hit amplitudes Observation of individual showers Line 2 operational in ~4 weeks
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