Peculiar velocities of galaxy clusters in a IllustrisTNG simulation based on mock observations of Sunyaev-Zel’dovich effects

Open Access

Fig. 3.

Radial profiles of the Compton y_tSZ parameter for the four mass bins of our sample. The radii are normalized to R₂₀₀ of the clusters. The lines represent the mean radial profile of y_tSZ, and the shaded regions indicate the scatter.

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