Fig. 9.

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Rescaled splashback radius as a function of the cluster peak height. The red solid curve and the corresponding shaded region represent the result of our reference fitting procedure model. The blue and orange curves correspond to the model predictions by More et al. (2015) and Diemer (2020), respectively. The different data points represent the relation measured by different authors, using various selected galaxy cluster samples and observables: galaxy projected correlation function (GP), weak lensing (WL), and in combination of weak and strong lensing (WL+SL) and stacked luminosity profiles (LP). X-ray, SZ and optically selected clusters are displayed using squares, triangles and crosses.
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