collaborators

12 papers

astro-ph.HE2026

Revealing massive black hole astrophysics: The potential of hierarchical inference with extreme mass-ratio inspiral observations

Shashwat Singh, Christian E. A. Chapman-Bird, Christopher P. L. Berry +1

The paper investigates how observations of extreme mass-ratio inspirals by LISA can be used with hierarchical Bayesian inference to measure massive black hole population properties…

gr-qc2026

Inference with finite time series II: the window strikes back

Colm Talbot, Sylvia Biscoveanu, Aaron Zimmerman +9

Smooth window functions are often applied to strain data when inferring the parameters describing the astrophysical sources of gravitational-wave transients. Within the LIGO-Virgo-…

gr-qc2026

GW231123: Overlapping Gravitational Wave Signals?

Qian Hu, Harsh Narola, Jef Heynen +4

The recently discovered gravitational wave event GW231123 was interpreted as the merger of two black holes with a total mass of 190-265 , making it the heaviest such merge…

gr-qc2026

Constraints on the extreme mass-ratio inspiral population from LISA data

Shashwat Singh, Christian E. A. Chapman-Bird, Christopher P L Berry +1

Gravitational waves from extreme mass-ratio inspirals (EMRIs), the inspirals of stellar-mass compact objects into massive black holes, are predicted to be observed by the Laser Int…

astro-ph.IM2026

Neural Bayesian updates to populations with growing gravitational-wave catalogs

Noah E. Wolfe, Matthew Mould, John Veitch +1

As gravitational-wave catalogs grow, they will become increasingly computationally expensive to analyze in their entirety, especially when inferring astrophysical source population…

gr-qc2025

Costs of Bayesian Parameter Estimation in Third-Generation Gravitational Wave Detectors: an Assessment of Current Acceleration Methods

Qian Hu, John Veitch

Bayesian inference with stochastic sampling has been widely used to obtain the properties of gravitational wave (GW) sources. Although computationally intensive, its cost remains m…