Citation notice #4072 · 2026-07-11 03:19:06.079886+00:00
The first decade of gravitational-wave measurements of black hole spins
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cites Two-harmonic approximation for gravitational waveforms from precessing binaries.Phys, which carries a correction notice dated 2020-07-17. One-hop deterministic notice: the citation edge exists in the Pith bibliography graph; no model judged whether the citation was load-bearing.
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01Evidence
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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
02Event
- Type
- Correction
- Source
- Crossref
- Original DOI
- 10.1103/physrevd.102.024055
- Notice DOI
- 10.1103/physrevd.102.024055
- Date
- 2020-07-17
- Title
- Two-harmonic approximation for gravitational waveforms from precessing binaries
- Reasons
- ['Correction']
- Work
- Two-harmonic approximation for gravitational waveforms from precessing binaries.Phys (1908) Physical review. D/Physical review. D.
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