activity
20242026
collaborators

6 papers

gr-qc2026

Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses

Charlie Hoy

The growing number of gravitational-wave (GW) observations allows for constraints to be placed on the underlying population of black holes; current estimates show that black hole s…

gr-qc2026

Leveraging rapid parameter estimates for efficient gravitational-wave Bayesian inference via posterior repartitioning

Metha Prathaban, Charlie Hoy, Michael J. Williams

Gravitational-wave astronomy typically relies on rigorous, computationally expensive Bayesian analyses. Several methods have also been developed to perform rapid, approximate Bayes…

hep-ex2026

Constraining the neutron star-black hole merger rate

Ian Harry, Charlie Hoy

Current template-based gravitational-wave searches for compact binary mergers neglect the general relativistic phenomenon of spin-induced orbital precession. Owing to their asymmet…

gr-qc2025

The Missing Multipole Problem: Investigating biases from model starting frequency in gravitational-wave analyses

Ryan Ursell, Charlie Hoy, Ian Harry +1

Our ability to infer the true source properties of colliding black holes from gravitational wave observations requires not only accurate waveform models but also their correct use.…

hep-ex2024

Premerger observation and characterization of massive black hole binaries

Gareth Cabourn Davies, Ian Harry, Michael J. Williams +11

We demonstrate an end-to-end technique for observing and characterizing massive black hole binary signals before they merge with the LISA space-based gravitational-wave observatory…

gr-qc2024

A rapid multi-modal parameter estimation technique for LISA

Charlie Hoy, Connor Weaving, Laura K. Nuttall +1

The Laser Interferometer Space Antenna (LISA) will observe gravitational-wave signals from a wide range of sources, including massive black hole binaries. Although numerous techniq…