Fig. 6.
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Left panel: mass-radius relation for the three EoS that we use in this work DD2 (Typel et al. 2010), SFHo (Steiner et al. 2013) and LS220 (Lattimer & Swesty 1991). We also include radii constraints from GW170817 (Bauswein et al. 2017; Annala et al. 2018) and NICER (Miller et al. 2019b). Right panel: values of chirp mass as a function of mass ratio q and the largest of the NS masses, M1.
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