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Böhm, Vanessa (2017): Cosmic lensing of galaxies and the cosmic microwave background beyond the linear regime. Dissertation, LMU München: Fakultät für Physik

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Figure 1.1:CMB temperature power spectrum DTTl= l(l + 1)CTTl/(2π) from the Planck2015 data release [184]
Figure 1.2:A sketch of the relevant angles in a lensing event: Two light rays (green andblack solid lines) are emitted at the source plane at distance χ and arrive at the observerseparated by an angle θ
Figure 1.4:Realizations of an unlensed CMB map (left panel) and a lensing potential(middle panel) on a sky cut of size (8.5 × 8.5)deg2.Lensing the CMB map with thedeflection field obtained from the lensing potential yields a lensed CMB field which is notshown
Figure 1.5:CMB power spectrum in a standard ΛCDM Universe before and after lensingby large-scale structure (computed with the publicly available CLASS code [23])
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Effect of weak Lensing by Large-Scale Structure on Galaxy Shapes Why study weak Lensing by Large-Scale Structure Implementation on the Sphere Summary and Conclusions The Effect of a non-vanishing Matter Bispectrum on standard Lensing Re- Prior Model Data Model Tests A: Simple Geometry Conclusions

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