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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 2.

Tangential shear, , as measured from all galaxies in the background galaxy catalogue for a zoomed-in view of the postage stamp. To reduce the noise, we have smoothed with a Gaussian with standard deviation 1  h −1 Mpc. The location of the mask is shown by the dashed circle.

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