Erratum: Post-Newtonian, quasicircular binary inspirals in quadratic modified gravity [Phys. Rev. D85, 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.