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arxiv: 1402.0053 · v1 · submitted 2014-02-01 · 🌀 gr-qc · astro-ph.IM

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Physically motivated exploration of the extrinsic parameter space in ground-based gravitational-wave astronomy

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classification 🌀 gr-qc astro-ph.IM
keywords gravitational-waveparameterbinarycoalescencecompactefficientspaceastronomy
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Efficient parameter estimation is critical for Gravitational-Wave astronomy. In the case of compact binary coalescence, the high dimensional parameter space demands efficient sampling techniques - such as Markov chain Monte Carlo (MCMC). A number of degeneracies effectively reduce the dimensionality of the parameter space and, when known, can render sampling algorithms more efficient with problem-specific improvements. We present in this paper an analytical description of a degeneracy involving the extrinsic parameters of a compact binary coalescence gravitational-wave signal, when data from a three detector network (such as Advanced LIGO/Virgo) is available. We use this new formula to construct a jump proposal, a framework for a generic sampler to take advantage of the degeneracy. We show the gain in efficiency for a MCMC sampler in the analysis of the gravitational-wave signal from a compact binary coalescence.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy

    astro-ph.IM 2018-11 accept novelty 5.0

    Bilby introduces a user-friendly Python library for accurate Bayesian inference on gravitational-wave signals from compact binaries and other sources, including hierarchical population modeling.