Modelling the selection of galaxy groups with end-to-end simulations

Open Access

Fig. 3.

Emission measure profiles with self-similar scaling, colour-coded for temperature, as a function of radius in units of R_500c. The units on the y-axis are Mpc keV^−1/2 cm⁻⁶. The bottom part of the panel shows the evolution of the intrinsic scatter of the profile at different radii. For reference, it is compared to the model from Comparat et al. (2020) and profiles of X-COP clusters (Ghirardini et al. 2019).

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