Figure 6 from A Detection of Dark Matter Halo Ellipticity using Galaxy Cluster Lensing in the SDSS

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A Detection of Dark Matter Halo Ellipticity using Galaxy Cluster Lensing in the SDSS

Authors: Anna Kathinka Dalland Evans and Sarah Bridle

EVANS & BRIDLE 2009 The Astrophysical Journal 695 1446.

Provider: AAS Journals

Caption: Figure 6.

Contours show output axis ratios for simulated misalignments between the light and dark matter. Axes show the input axis ratio f _in and standard deviation σ _θ (in degrees) of the angle distribution of the simulated clusters.

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