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Reference changes · DOI
Two-harmonic approximation for gravitational waveforms from precessing binaries.Phys
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Crossref
2 open · 2 total · 0 disputed
- Event date
- 2020-07-17
01One-hop citing occurrences
Correction
Open
GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$
ref [155] ·
2507.08219
· notice #4071
· dispute
Raw extraction · bibliography line
Fairhurst, Stephen and Green, Rhys and Hoy, Charlie and Hannam, Mark and Muir, Alistair. Two-harmonic approximation for gravitational waveforms from precessing binaries. Phys. Rev. D. 2020. doi:10.1103/PhysRevD.102.024055. arXiv:1908.05707
Correction
Open
The first decade of gravitational-wave measurements of black hole spins
ref [164] ·
2606.06209
· notice #4072
· dispute
Raw extraction · citation context
higher-order multipoles and variations occurring on the precessional timescale have been proposed [160,161]. Alternatively, the measurability of precession can be captured via the precessing signal-to-noise ratio (SNR), by decomposing the waveform into a series of non-precessing harmonics that beat against each other to generate the amplitude and phase modulations imprinted by precession [162-164]. 3.2. Measurability of spin in individual events The spins of compact-object binaries are measured using Bayesian inference, by com- paring the GW strain data to waveforms h(⃗θ) from across the parameter space of interest. Stochastic sampling techniques are used to obtain samples from the posterior probability distribution on the binary parameters, where the likelihood of observing frequency-domain