Figure 4 from Halo Pressure Profile through the Skew Cross-power Spectrum of the Sunyaev–Zel’dovich Effect and CMB Lensing in Planck

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Halo Pressure Profile through the Skew Cross-power Spectrum of the Sunyaev–Zel’dovich Effect and CMB Lensing in Planck

Authors: Nicholas Timmons, Asantha Cooray, Chang Feng, and Brian Keating

2017 The Astrophysical Journal Letters 849 L6.

Provider: AAS Journals

Caption: Figure 4.

Best-fit model of the gas pressure P_e(r) including the 1σ confidence region shown by the shaded region. For comparison the pressure profiles measured in Planck Collaboration et al. (2013), Arnaud et al. (2010), and Sayers et al. (2013) are also shown as a 1σ region. The pressure profiles have been set to z = 0 for comparison.

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