Open Access

Fig. A.2

image

Radius against mass from terrestrial mass planets up to massive stars. Data are taken from the exoplanets.org catalog, Malkov (2007), and Torres et al. (2010). The red solid line represents the continuous model, comprised of Bashi et al. (2017) from 10−6 to 0.004 M, Baraffe et al. (2003) from 0.004 to 0.1 M, BT-settl from 0.1 to 1.1 M, and the empirical relation RM0.57 above 1.1 M (e.g., Demircan & Kahraman 1991).

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