Post-Newtonian, quasicircular binary inspirals in quadratic modified gravity (vol 85, 064022, 2012)

In this erratum, we point out that the correction to the gravitational energy flux from compact binary inspirals in dynamical Chern-Simons gravity enters at third post-Newtonian order instead of second post-Newtonian order. We also correct the scalar energy flux at second post-Newtonian order by considering terms that we missed in the original paper.