Laue Gamma-Ray Lenses for Space Astrophysics: Status and Prospects
Figure 20
(a) Difference between the PSF measured and that obtained with a Monte Carlo code by assuming a perfect positioning of the crystal tiles in the lens. (b) Cumulative distribution of the focused photons as a function of radial distance from the focal point. Black line: expected distribution in the case of a perfect positioning of the crystal tiles in the lens. Red line: measured distribution. Reprinted from [34].
