Erratum: Gravitational Waves from Quasicircular Black-Hole Binaries in Dynamical Chern-Simons Gravity [Phys. Rev. Lett. 109, 251105 (2012)]

Figure 1

Projected $1\sigma$ constraints on ${\xi }^{1/4}$ in km with the second-generation ground-based detectors (top left), ET (top right), DECIGO/BBO (bottom left), and LISA (bottom right) for black-hole binaries with $m_1/m_2=2$. The fixed values for ${\chi }_1$ and $D_L$ are shown at the top right of each panel. The constraints using the second-generation ground-based detectors have been obtained by assuming that the spins are known a priori. This roughly models projected constraints with precessing black-hole binary observations and may be correct within an error of 30%. For other detectors, binaries are assumed to be spin aligned (or antialigned). The colored contours show the regions of parameter space where the constraints on ${\xi }^{1/4}$ also satisfy $\mathrm{\Delta }{\zeta }^{\prime }<1$; thus, the small coupling approximation is satisfied at the fiducial luminosity distances chosen.