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Erratum: Post-Newtonian diagnostic of quasiequilibrium binary configurations of compact objects [Phys. Rev. D<b>69</b>, 104021 (2004)]
Using equations of motion accurate to the third post-Newtonian (3PN) order (O(v/c) 6 beyond Newtonian gravity), we derive expressions for the total energy E and angular momentum J of the orbits of compact binary systems (black holes or neutron stars) for arbitrary orbital eccentricity.We also incorporate finite-size contributions such as …