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The spin-free binary-inspiral parameter-space introduced by Tanaka andTagoshi to construct a uniformly-spaced lattice of templates at (and possiblybeyond) $2.5PN$ order is shown to work for all first generation interferometricgravitational wave antennas. This allows to extend the minimum-redundantcardinal interpolation techniques of the correlator bank developed by theAuthors to the highest available order PN templates. The total number of 2PNtemplates to be computed for a minimal match $\Gamma=0.97$ is reduced by afactor 4, as in the 1PN case.Comment: 9 pages, 8 figures, 3 tables, accepted for publication in Phys. Rev.

physical review. d. particles, fields, gravitation, and cosmology/physical review. d. particles and fields

Tanaka-Tagoshi parametrization of post-first-post-Newtonian spin-free gravitational wave chirps: Equispaced and cardinal interpolated lattices for first generation interferometric antennas