Virial quantities of galaxy clusters from extrapolating strong-lensing mass profiles

Open Access

Fig. 4.

Scaling relation between the total mass from the Hernquist profile, $M_{H}^{tot}$ $M_{\mathrm{H}}^{\mathrm{tot}}$ , and the M_200c values from the literature (Jee et al. 2014; Medezinski et al. 2016; Umetsu et al. 2018). On the left, we show the linear best fit with the solid line together with its corresponding 1σ shaded zone. On the right, we show the best-fit power law of the relation with the solid line and its respective shaded zone.

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