Mohamad-Ziad Charif - Antares

Figure 5.12: Comparison between the Sun’s Cos[θ] extracted from data, Scrambleddata, and Monte Carlo neutrino/muon. It shows the normalized distributionswith respect to the lifetime without any quality cuts. The top distributions are forthe 10pe periods, and the bottom are for the 3pe, and from left to right: 5, 9, 10,12 Lines detector.cone centered around the Sun as it follows it around the sky during our livetime.A good agreement can be found between the scrambled data and the Monte Carlo.With χ 2 < 2 selection the event sample is largely dominated by atm µ events, ascan be seen in figure 5.9. In addition, for small ∆(Ψ) angle (which is the halfconeangle), the distribution in figure 5.15 is compatible with random distributionof events ∝ θ 2 .89