Auger North - Fermilab Center for Particle Astrophysics

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<strong>Auger</strong> South! Observed the GZK feature in the spectrum! Determined Sky anisotropies > 60 EeV! Showed that the GZK sphere is populated! Strongest UHE tau neutrino and UHE photon limits!
<strong>Auger</strong> South! Observed the GZK feature in the spectrum! Determined Sky anisotropies > 60 EeV! Showed that the GZK sphere is populated! Strongest UHE tau neutrino and UHE photon limits!
Page 1 and 2: The Pierre Auger Observatory Auger
Page 3 and 4: To Discover UHECR Sources ! need:!
Page 5: Auger South!
Page 9 and 10: Attenuation length! e + e - π Atte
Page 11 and 12: Horizons:! 10 19 eV ~ 1 Gpc! 100 Mp
Page 14 and 15: Recent Auger Spectrum!
Page 16 and 17: Auger South! Observed the GZK featu
Page 18 and 19: Auger VCV correlation! 27 events te
Page 20 and 21: First 27 events!
Page 22 and 23: UHE neutrino limit!
Page 26 and 27: Composition observable: ! shower ma
Page 28 and 29: Puzzling Composition! Unexpected As
Page 30 and 31: Neutrino Fluxes!
Page 32 and 33: Above 60 EeV: ! either Protons or I
Page 34 and 35: If Correlated with sources ! < 10 o
Page 36 and 37: Hadronic Interactions ! Parameters
Page 40 and 41: Auger North - 10 yr Auger South - 1
Page 42 and 43: FD disentangle Composition !
Page 44 and 45: Galactic Plane!
Page 46 and 47: Determine Source Distribution! Type
Page 48 and 49: Lindsleys Exposure Evolution - Line
Page 50 and 51: Auger North Objectives! Obtain the
Page 52 and 53: State of Colorado Auger North: 4000
Page 54 and 55: Features of Auger North Fluorescenc
Page 56 and 57:
Communications System Campus Area M
Page 58 and 59:
Argentina " "Netherlands! Australia
Page 60 and 61:
Estimated Construction Cost! WBS Ac
Page 62 and 63:
Funding! Auger South ($54M):! Europ
Page 64 and 65:
US Auger Groups! Argonne National L
Page 66 and 67:
The Pierre Auger Observatory Auger
Page 68 and 69:
Auger North Auger South Auger North
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Auger North - Fermilab Center for Particle Astrophysics

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