papers

Publications (7)

astro-ph.CO2012

The strongest gravitational lenses: I. The statistical impact of cluster mergers

Matthias Redlich, Matthias Bartelmann, Jean-Claude Waizmann +1

For more than a decade now, it has been controversial whether or not the high rate of giant gravitational arcs and the largest observed Einstein radii are consistent with the stand…

astro-ph.CO2014

Consistent use of Type Ia supernovae highly magnified by galaxy clusters to constrain the cosmological parameters

Adi Zitrin, Matthias Redlich, Tom Broadhurst

We discuss how Type Ia supernovae (SNe) strongly magnified by foreground galaxy clusters should be self-consistently treated when used in samples fitted for the cosmological parame…

astro-ph.CO2015

Evolution of linear perturbations in Lemaître-Tolman-Bondi void models

Sven Meyer, Matthias Redlich, Matthias Bartelmann

We study the evolution of linear perturbations in a Lemaître-Tolman-Bondi (LTB) void model with realistic cosmological initial conditions. Linear perturbation theory in LTB models…

astro-ph.CO2014

Probing spatial homogeneity with LTB models: a detailed discussion

Matthias Redlich, Krzysztof Bolejko, Sven Meyer +2

Do current observational data confirm the assumptions of the cosmological principle, or is there statistical evidence for deviations from spatial homogeneity on large scales? To ad…

astro-ph.CO2014

The strongest gravitational lenses: IV. The order statistics of the largest Einstein radii with cluster mergers

Matthias Redlich, Jean-Claude Waizmann, Matthias Bartelmann

Based on techniques developed in the previous papers of this series, we investigate the impact of galaxy-cluster mergers on the order statistics of the largest Einstein radii. We s…

astro-ph.CO2014

The strongest gravitational lenses: III. The order statistics of the largest Einstein radii

Jean-Claude Waizmann, Matthias Redlich, Massimo Meneghetti +1

The Einstein radius (ER) of a gravitational lens encodes information about decisive quantities such as halo mass, concentration, triaxiality, and orientation with respect to the ob…