Mohamad-Ziad Charif - Antares
Mohamad-Ziad Charif - Antares Mohamad-Ziad Charif - Antares
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12.07.2015
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Figure 3.29: Comparison between sky visibility in galactic coordinates of ICE-CUBE (left) and ANTARES (right).62
Figure 3.30: Effective area at trigger level for the neutrinos as a function ofLog 10 (neutrino energy).63
- Page 14 and 15: Figure 2.5: Combination of the WMAP
- Page 17: Figure 2.6: Temporal evolution of t
- Page 20 and 21: Figure 2.9: Parameter space of m 1/
- Page 22 and 23: Figure 2.10: Limits on spin-indepen
- Page 26 and 27: Figure 2.14: Detected gamma ray flu
- Page 28 and 29: 600km/s. If we assume the worst cas
- Page 30 and 31: Figure 2.17: Conversion factor from
- Page 32 and 33: The eigenstate mixing can be writte
- Page 34 and 35: Figure 2.19: Flux of ν µ / ¯ν
- Page 36 and 37: Figure 3.1: The neutral current (NC
- Page 38 and 39: Muon Energy (GeV )1p| dEdx | (GeV.c
- Page 40 and 41: Figure 3.4: Energy loss of per dist
- Page 42 and 43: Figure 3.6: Effective muon range as
- Page 44 and 45: Figure 3.8: Differential flux of at
- Page 46 and 47: 3.2.1.1 Detector layoutOptical Modu
- Page 48 and 49: • The LED (light emitting diode)
- Page 50 and 51: Anchor & BuoyEach line is anchored
- Page 52 and 53: Figure 3.17: Distribution of azimut
- Page 54 and 55: Figure 3.20: Height and radial disp
- Page 56 and 57: Figure 3.22: Distribution of sea cu
- Page 58 and 59: Figure 3.24: Time offset among OMs
- Page 60 and 61: Figure 3.26: Distribution of time d
- Page 62 and 63: Line number Connection Date Mainten
- Page 66 and 67: Figure 3.31: The effective area for
- Page 68 and 69: Figure 4.1: Median counting rate of
- Page 70 and 71: Figure 4.4: Average neutrino events
- Page 72 and 73: 2. All hits on the same floor are m
- Page 74 and 75: 4.2.1 Neutrino simulationFigure 4.6
- Page 76 and 77: • Multiplicity range of the muon
- Page 78 and 79: Chapter 5Dark Matter search in the
- Page 80 and 81: Figure 5.2: Annihilation spectrum f
- Page 82 and 83: Livetime(days) 5 Lines 9 Lines 10 L
- Page 84 and 85: Figure 5.4: Monte Carlo Truth distr
- Page 86 and 87: Figure 5.7: Tchi2 distribution for
- Page 88 and 89: Figure 5.9: Tchi2 distribution for
- Page 90 and 91: Figure 5.11: Sun’s position taken
- Page 92 and 93: Figure 5.13: Comparison between the
- Page 94 and 95: Figure 5.15: Estimation of the back
- Page 96 and 97: Figure 5.16: Mean angle between the
- Page 98 and 99: Figure 5.18: A comparison of the di
- Page 100 and 101: a look at figure 5.22 we find a cle
- Page 102 and 103: The resulting optimized sensitiviti
- Page 104 and 105: Figure 5.26: A comparison plot of t
- Page 106 and 107: dΦ µdE ν= dΦ νdE νP earth ρN
- Page 108 and 109: Figure 5.31: Limits on the muon flu
- Page 110 and 111: Chapter 6Dark Matter search in the
- Page 112 and 113: Figure 6.1: . True Position of the
Figure 3.30: Effective area at trigger level for the neutrinos as a function ofLog 10 (neutrino energy).63
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