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Does Matter Matter? Using the Mass Distribution to Distinguish Neutron Stars and Black Holes

  • Authors: Maya Fishbach, Reed Essick, and Daniel E. Holz

2020 The Astrophysical Journal Letters 899 L8.

  • Provider: AAS Journals

Caption: Figure 6.

Joint posterior on the power-law slopes α1 (NS mass range) and α2 (BH mass range) for the full POWER LAW + DIP + BREAK model (green). The two-dimensional contours show 50% and 90% credible regions, while vertical dashed lines show one-dimensional 90% credible intervals. For comparison, we show the power-law slope inferred under the POWER-LAW fit to (blue) only the BBH and (orange) all GWTC-1 events. We recover α1 < α2 with 91% credibility; α1 = α2 in this model reduces to the POWER LAW + DIP model.

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