Fig. 12
Left: Kolmogorov-Smirnov distance d and Monte-Carlo simulations for the two assumed alternative distributions of polar axes. Top: uniform distribution of βs between ±90° (i.e. spin axes in ecliptic plane). Bottom: all objects with β = 0° (i.e. spin axes perpendicular ecliptic plane). In each case, the K-S distance to the data is plotted (left panels) as a function of Γ for the four roughness cases. Right panels show Monte-Carlo simulations for the random roughness cases.
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