Fig. C.1.
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Comparison of our neutron star mass distribution posterior (power law model) with the GWTC-3 result from the population study described in Abbott et al. 2021a (their POWER model). Shaded areas show the 90% and 50% credible regions, while thick solid lines show the medians. Red is for our result (Sect. 4.2), blue is for the GWTC-3.
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