activity
20232026
most citedCalibrating approximate Bayesian credible intervals of gravitational-wave parameters

2 citations · 2 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2026

Variational Bayesian Inference for the Spectral Structure of LISA Noise

Jianan Liu, Avi Vajpeyi, Renate Meyer +2

Estimating spectral density matrices for future space-based gravitational-wave detectors such as LISA is challenging due to the long duration of the data and the correlated instrum…

gr-qc2026

Bayesian P-spline recovery of stochastic gravitational-wave backgrounds in LISA

Nazeela Aimen, Patricio Maturana-Russel, Avi Vajpeyi +2

The detection of a stochastic gravitational-wave background (SGWB) is a primary science objective for the Laser Interferometer Space Antenna (LISA). However, extracting these signa…

astro-ph.HE2026

Insights into the Pulsar Timing Array hypothesis space

El Mehdi Zahraoui, Patricio Maturana-Russel, Willem van Straten +2

We present novel insights into the pulsar-noise model space in pulsar timing array (PTA) experiments. Through a comparative analysis of the same Parkes PTA second data release obse…

gr-qc2026

Bayesian nonparametric estimation of correlated gravitational wave detector network noise using matrix-gamma process priors

Yixuan Liu, Renate Meyer, Nelson Christensen +4

This paper addresses the important problem of estimating the noise spectral density of next-generation gravitational-wave detectors, such as LISA and the Einstein Telescope (ET), w…

stat.ME2026

Multivariate Bayesian P-spline estimation of spectral density matrices, with application to LISA TDI noise

Avi Vajpeyi, Renate Meyer, Patricio Maturana-Russel +1

We present a Bayesian P-spline method for estimating the frequency-dependent cross-spectral density matrix of stationary multivariate time series. The inverse spectral matrix is pa…

astro-ph.IM2025

Enhancing evidence estimation through informed probability density approximation

El Mehdi Zahraoui, Patricio Maturana-Russel, Avi Vajpeyi +3

We introduce the Morph approximation, a class of product approximations of probability densities that selects low-order disjoint parameter blocks by maximizing the sum of their tot…

gr-qc2025

Bayesian power spectral density estimation for LISA noise based on penalized splines with a parametric boost

Nazeela Aimen, Patricio Maturana-Russel, Avi Vajpeyi +2

Flexible and accurate noise characterization is crucial for the precise estimation of gravitational-wave parameters. We introduce a Bayesian method for estimating the power spectra…

astro-ph.IM2024

Generalized Steppingstone Sampling: Efficient marginal likelihood estimation in gravitational wave analysis of Pulsar Timing Array data

El Mehdi Zahraoui, Patricio Maturana-Russel, Willem van Straten +2

Globally, Pulsar Timing Array (PTA) experiments have revealed evidence supporting an existing gravitational wave background (GWB) signal in the PTA data set. Apart from acquiring m…

gr-qc2024

Variational inference for correlated gravitational wave detector network noise

Jianan Liu, Avi Vajpeyi, Renate Meyer +5

Gravitational wave detectors like the Einstein Telescope and LISA generate long multivariate time series, which pose significant challenges in spectral density estimation due to a…

gr-qc2023★ 2 cited

Calibrating approximate Bayesian credible intervals of gravitational-wave parameters

Ruiting Mao, Jeong Eun Lee, Ollie Burke +3

Approximations are commonly employed in realistic applications of scientific Bayesian inference, often due to convenience if not necessity. In the field of gravitational-wave (GW)…

astro-ph.HE2023

Inference of proto-neutron star properties in core-collapse supernovae from a gravitational-wave detector network

T. Bruel, M-A. Bizouard, M. Obergaulinger +6

The next Galactic core-collapse supernova (CCSN) will be a unique opportunity to study within a fully multi-messenger approach the explosion mechanism responsible for the formation…