Observational constraints on the optical and near-infrared emission from the neutron star–black hole binary merger candidate S190814bv

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Fig. 13.

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Constraints on the BH spin (a_BH) and the BH mass (M_BH) of the NS–BH binary, assuming remnant disc and tidal ejecta mass limits of M_disc < 0.3 M_⊙ and M_t < 10⁻² M_⊙, which correspond to approximately 1 sigma exclusion confidence (see text). The SFHo EoS has been adopted to compute the NS tidal deformability.

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