Figure 9 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 9.

Subaru S/N map obtained by 1000 bootstraps of the Subaru source catalog. The signal is the original convergence map, and the noise is determined from the standard deviation of the bootstrapped convergence maps. The peak of the mass distribution is detected at ﹩9\sigma ﹩ significance, and the substructures to the NW and SE are detected at ﹩3\sigma ﹩ significance.

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