Erratum: Post-Newtonian diagnostic of quasiequilibrium binary configurations of compact objects [Phys. Rev. D 69, 104021 (2004)]

1.

Conservative self-force correction to the innermost stable circular orbit: Comparison with multiple post-Newtonian-based methods
Marc Favata
Phys. Rev. D 83, 024027 (2011)

2.

Intrinsic and extrinsic geometries of a tidally deformed black hole
Ian Vega, Eric Poisson, Ryan Massey
Classical and Quantum Gravity 28, 175006 (2011)

3.

Effective one body description of tidal effects in inspiralling compact binaries
Thibault Damour and Alessandro Nagar
Phys. Rev. D 81, 084016 (2010)

4.

Relativistic tidal properties of neutron stars
Thibault Damour and Alessandro Nagar
Phys. Rev. D 80, 084035 (2009)

5.

Initial data for black hole–neutron star binaries: A flexible, high-accuracy spectral method
Francois Foucart, Lawrence E. Kidder, Harald P. Pfeiffer, and Saul A. Teukolsky
Phys. Rev. D 77, 124051 (2008)

6.

Nonrotating black hole in a post-Newtonian tidal environment
Stephanne Taylor and Eric Poisson
Phys. Rev. D 78, 084016 (2008)

7.

Effective field theory of gravity for extended objects
Walter D. Goldberger and Ira Z. Rothstein
Phys. Rev. D 73, 104029 (2006)