We present a new frequency-domain phenomenological model of the gravitational-wave
signal from the inspiral, merger and ringdown of nonprecessing (aligned-spin) black-hole …

In this paper we discuss the anatomy of frequency-domain gravitational-wave signals from
nonprecessing black-hole coalescences with the goal of constructing accurate …

The construction of a model of the gravitational-wave (GW) signal from generic
configurations of spinning-black-hole binaries, through inspiral, merger, and ringdown, is …

We present the first analytical inspiral-merger-ringdown gravitational waveforms from binary
black holes (BBHs) with nonprecessing spins, that is based on a description of the late …

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

We compare the science capabilities of different eLISA mission designs, including four-link
(two-arm) and six-link (three-arm) configurations with different arm lengths, low-frequency …

Gravitational waves (GWs) emitted by generic black-hole binaries show a rich structure that
directly reflects the complex dynamics introduced by the precession of the orbital plane …

OBJECTIVE To test the hypothesis that vitamin D receptor polymorphism is associated with
calcific aortic valve stenosis. DESIGN The distribution of one polymorphism of the vitamin D …

The detections of gravitational-wave (GW) signals from compact binary coalescence by
ground-based detectors have opened up the era of GW astronomy. These observations …

Gravitational-wave observations of binary black holes currently rely on theoretical models
that predict the dominant multipoles (ℓ= 2,| m|= 2) of the radiation during inspiral, merger …