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Table B.1.

Summary of median and 90% credible intervals of 200114_020818 for different waveform models. The columns show the waveform model used for parameter estimation, the source frame component masses mi, effective spin parameters χeff and χp, luminosity distance DL, the angle between the total angular momentum and the direction of propagation of the gravitational wave signal θJN, and the log10Bayes Factor between the signal and Gaussian noise given the model.

Waveform Model m1 (M) m2 (M) χeff χp DL (Mpc) θJN log10BSN
IMRPhenomXPHM 197 . 2 31.2 + 22.6 $ 197.2^{+22.6}_{-31.2} $ 62 . 1 16.6 + 11.1 $ 62.1^{+11.1}_{-16.6} $ 0 . 3 0.2 + 0.1 $ -0.3^{+0.1}_{-0.2} $ 0 . 6 0.2 + 0.1 $ 0.6^{+0.1}_{-0.2} $ 593 . 4 146.7 + 276.8 $ 593.4^{+276.8}_{-146.7} $ 0 . 9 0.3 + 0.8 $ 0.9^{+0.8}_{-0.3} $ 24.9
SEOBNRv4PHM 179 . 6 60.4 + 17.1 $ 179.6^{+17.1}_{-60.4} $ 26 . 7 6.4 + 7.3 $ 26.7^{+7.3}_{-6.4} $ 0 . 7 0.1 + 0.2 $ -0.7^{+0.2}_{-0.1} $ 0 . 2 0.2 + 0.3 $ 0.2^{+0.3}_{-0.2} $ 475 . 6 153.0 + 199.1 $ 475.6^{+199.1}_{-153.0} $ 1 . 6 1.1 + 1.2 $ 1.6^{+1.2}_{-1.1} $ 26.2
NRSur7dq4 75 . 0 18.8 + 32.9 $ 75.0^{+32.9}_{-18.8} $ 42 . 5 18.0 + 16.4 $ 42.5^{+16.4}_{-18.0} $ 0 . 5 0.2 + 0.3 $ -0.5^{+0.3}_{-0.2} $ 0 . 5 0.3 + 0.3 $ 0.5^{+0.3}_{-0.3} $ 1797 . 0 1027.0 + 1601.0 $ 1797.0^{+1601.0}_{-1027.0} $ 2 . 0 1.6 + 0.9 $ 2.0^{+0.9}_{-1.6} $ 22.3

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