The article provides ready-to-use first post-Newtonian-accurate frequency-domain gravitational wave forms for eccentric nonspinning compact binaries of arbitrary mass ratio including the first post-Newtonian point particle corrections to the far-zone gravitational wave amplitude, given in terms of tensor-spherical harmonics. The averaged equations for the decay of the eccentricity and growth of radial frequency due to radiation reaction are used to provide stationary phase approximations to the frequency-domain wave forms.
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