Figure 3 from Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 deg2 SPT-SZ Survey

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Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 deg2 SPT-SZ Survey

Authors: Z. Hou, C. L. Reichardt, K. T. Story, B. Follin, R. Keisler, K. A. Aird, B. A. Benson, L. E. Bleem, J. E. Carlstrom, C. L. Chang, H.-M. Cho, T. M. Crawford, A. T. Crites, T. de Haan, R. de Putter, M. A. Dobbs, S. Dodelson, J. Dudley, E. M. George, N. W. Halverson, G. P. Holder, W. L. Holzapfel, S. Hoover, J. D. Hrubes, M. Joy, L. Knox, A. T. Lee, E. M. Leitch, M. Lueker, D. Luong-Van, J. J. McMahon, J. Mehl, S. S. Meyer, M. Millea, J. J. Mohr, T. E. Montroy, S. Padin, T. Plagge, C. Pryke, J. E. Ruhl, J. T. Sayre, K. K. Schaffer, L. Shaw, E. Shirokoff, H. G. Spieler, Z. Staniszewski, A. A. Stark, A. van Engelen, K. Vanderlinde, J. D. Vieira, R. Williamson, and O. Zahn

Hou et al. 2014 The Astrophysical Journal 782 74.

Provider: AAS Journals

Caption: Figure 3.

Here we illustrate the degree of consistency between the CMB data and the two external data sets which are in the most tension: BOSS and H ₀. The solid lines mark the 1 and 2σ contours from the CMB data in the H ₀ − r _s / D _V (0.57) plane, while the color encodes the value of Ω _m h ², as shown in the color scale on the right. From left to right, the CMB data used is WMAP 7, SPT+τ, and SPT+ WMAP 7. The horizontal solid and dashed lines mark the central value and 1σ region for the BOSS BAO measurement, while the vertical lines do the same for H ₀. The joint 1 and 2σ likelihood regions for BOSS+ H ₀ measurements are denoted by the dark and light gray shaded contours.

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