Erratum: Binary Black Hole Mergers in the First Advanced LIGO Observing Run [Phys. Rev. X 6, 041015 (2016)]

Popular Summary

This is an Erratum, so has no Popular Summary.

Figure 1

This is the corrected Fig. 8 of [4], showing the 90% credible upper bounds on deviations in the PN coefficients from GW150914, from GW151226 and from both. It also fixes a previous plotting error for the 0 PN individual bounds (the GW150914 and GW151226 bounds were incorrectly drawn on top of eachother).

Figure 2

This is the corrected Fig. 7 of [4], showing the posterior density distributions and 90% credible intervals for the relative deviations PN parameters $p_i$, as well as intermediate parameters ${\beta }_i$ and merger-ringdown parameters ${\alpha }_i$. The corrected posterior for the 0.5 PN single-parameter analysis peaks below 0, while previously reported to peak above; the posterior is still consistent with GR.