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GW190521: Orbital Eccentricity and Signatures of Dynamical Formation in a Binary Black Hole Merger Signal

  • Authors: Isobel Romero-Shaw, Paul D. Lasky, Eric Thrane, and Juan Calderón Bustillo

2020 The Astrophysical Journal Letters 903 L5.

  • Provider: AAS Journals

Caption: Figure 2.

Results of SEOBNRE and IMRPHENOMPV2 analysis of simulated data using GW190521-like injections. Left: posterior distributions for eccentricity at 10 Hz for GW190521-like injection studies with varying e10 and ﹩{\chi }_{p}﹩, obtained using SEOBNRE. Right: posterior distribution for precession parameter ﹩{\chi }_{p}﹩ for GW190521-like injection studies with varying e10 and ﹩{\chi }_{p}﹩, recovered using IMRPHENOMPV2. The prior distributions are shown in gray.

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