2 Fast 2 Fiducial: Gaussian processes for the interpolation and marginalization of waveform error in extreme-mass-ratio-inspiral parameter estimation
arXiv:1912.11543 · doi:10.1103/PhysRevD.101.044027
Abstract
A number of open problems hinder our present ability to extract scientific information from data that will be gathered by the near-future gravitational-wave mission LISA. Many of these relate to the modeling, detection and characterization of signals from binary inspirals with an extreme component-mass ratio of . In this paper, we draw attention to the issue of systematic error in parameter estimation due to the use of fast but approximate waveform models; this is found to be relevant for extreme-mass-ratio inspirals even in the case of waveforms with overlap accuracy and moderate () signal-to-noise ratios. A scheme that uses Gaussian processes to interpolate and marginalize over waveform error is adapted and investigated as a possible precursor solution to this problem. Several new methodological results are obtained, and the viability of the technique is successfully demonstrated on a three-parameter example in the setting of the LISA Data Challenge.
arXiv commentPublished version
References in corpus (26)
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- The motion of point particles in curved spacetime
- Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals
- LISA Capture Sources: Approximate Waveforms, Signal-to-Noise Ratios, and Parameter Estimation Accuracy
- Angular Resolution of the LISA Gravitational Wave Detector
- Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries
- Science with the space-based interferometer LISA. IV: Probing inflation with gravitational waves
- Gravitational self force in extreme mass-ratio inspirals
- A Comparison of search templates for gravitational waves from binary inspiral
- Event rate estimates for LISA extreme mass ratio capture sources
- "Kludge" gravitational waveforms for a test-body orbiting a Kerr black hole
- Gravitational wave snapshots of generic extreme mass ratio inspirals
- LISA detections of massive black hole inspirals: parameter extraction errors due to inaccurate template waveforms
- A stochastic template placement algorithm for gravitational wave data analysis
- The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals
- LISACode : A scientific simulator of LISA
- Random template banks and relaxed lattice coverings
- Improved analytic extreme-mass-ratio inspiral model for scoping out eLISA data analysis
- Building a stochastic template bank for detecting massive black hole binaries
- An algorithm for detection of extreme mass ratio inspirals in LISA data
- Improving gravitational-wave parameter estimation using Gaussian process regression
- Novel Method for Incorporating Model Uncertainties into Gravitational Wave Parameter Estimates
- The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy
- Fast methods for training Gaussian processes on large data sets
- Global analysis for the LISA gravitational wave observatory
- Augmented kludge waveforms and Gaussian process regression for EMRI data analysis
Cited by in corpus (18)
- Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
- Distinguishing fuzzballs from black holes through their multipolar structure
- Extreme mass ratio inspirals with spinning secondary: a detailed study of equatorial circular motion
- Extreme mass-ratio inspirals around a spinning horizonless compact object
- Waveform accuracy and systematic uncertainties in current gravitational wave observations
- Detecting Gravitational-waves from Extreme Mass Ratio Inspirals using Convolutional Neural Networks
- Looking at Blazar Light Curve Periodicities with Gaussian Processes
- Non-local parameter degeneracy in the intrinsic space of gravitational-wave signals from extreme-mass-ratio inspirals
- Gravitational wave from extreme mass-ratio inspirals as a probe of extra dimensions
- Detecting Subsolar-Mass Primordial Black Holes in Extreme Mass-Ratio Inspirals with LISA and Einstein Telescope
- Model independent tests of the Kerr bound with extreme mass ratio inspirals
- Identification of Gravitational-waves from Extreme Mass Ratio Inspirals
- Bayesian parameter-estimation of Galactic binaries in LISA data with Gaussian Process Regression
- Assessing and marginalizing over compact binary coalescence waveform systematics with RIFT
- Testing the nature of dark compact objects with gravitational waves
- Testing gravity with Extreme-Mass-Ratio Inspirals
- Improving the scalability of Gaussian-process error marginalization in gravitational-wave inference
- Calibrating approximate Bayesian credible intervals of gravitational-wave parameters