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The gravitational radiation from point particle binaries is computed at thethird post-Newtonian (3PN) approximation of general relativity. Threepreviously introduced ambiguity parameters, coming from the Hadamard self-fieldregularization of the 3PN source-type mass quadrupole moment, are consistentlydetermined by means of dimensional regularization, and proved to have thevalues xi = -9871/9240, kappa = 0 and zeta = -7/33. These results complete thederivation of the general relativistic prediction for compact binary inspiralup to 3.5PN order, and should be of use for searching and deciphering thesignals in the current network of gravitational wave detectors.Comment: 4 pages in 2-column format, LaTeX 2e, REVTeX 4, no figur

Gravitational Radiation from Inspiralling Compact Binaries Completed at the Third Post-Newtonian Order