Figure 12 from MC2: Subaru and Hubble Space Telescope Weak-lensing Analysis of the Double Radio Relic Galaxy Cluster PLCK G287.0+32.9

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MC²: Subaru and Hubble Space Telescope Weak-lensing Analysis of the Double Radio Relic Galaxy Cluster PLCK G287.0+32.9

Authors: Kyle Finner, M. James Jee, Nathan Golovich, David Wittman, William Dawson, Daniel Gruen, Anton M. Koekemoer, Brian C. Lemaux, and Stella Seitz

2017 The Astrophysical Journal 851 46.

Provider: AAS Journals

Caption: Figure 12.

SIS and NFW halo fits to the reduced tangential shear. The radial profile is measured from the BCG. High S/N extending to large radii permits a two-parameter NFW profile fit. Galaxies within ﹩100^{\prime\prime} ﹩ are excluded from the fitting algorithm to omit the central area where the weak-lensing approximation may break down.

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