Fig. 10.

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Top panel: Mdd as a function of NS radius from NR runs due to Radice et al. (2018) and Nedora et al. (2021) having q ≃ 1. Bottom panel: log(Lpeak[erg s−1]) for an equatorial orientation as a function of primary mass M1, for runs in Table 1 also having q ≃ 1. We also indicate a conservative lower limit estimate of equatorial peak luminosity for a GW170817-like transient.
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