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20082026
most citedFrequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era

1.1k citations · 7.4k across the 52 of their papers we have counts for

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gr-qc2010★ 49 cited

Length requirements for numerical-relativity waveforms

Mark Hannam, Sascha Husa, Frank Ohme +1

One way to produce complete inspiral-merger-ringdown gravitational waveforms from black-hole-binary systems is to connect post-Newtonian (PN) and numerical-relativity (NR) results…

gr-qc2010★ 498 cited

Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries

L. Santamaria, F. Ohme, P. Ajith +10

We present a new phenomenological gravitational waveform model for the inspiral and coalescence of non-precessing spinning black hole binaries. Our approach is based on a frequency…