activity
20242026
most citedBuilding a bridge between comparable and extreme mass ratio black hole binaries: a single spin precessing model for the final state

5 citations · 5 across the 5 of their papers we have counts for

collaborators

5 papers

gr-qc2026

Parity symmetry as a diagnostic for spin-precessing binary-black-hole waveform models

Héctor Estellés, Sascha Husa, Eleanor Hamilton +3

Parity invariance of general relativity imposes exact relations between waveforms and remnant properties of binary-black-hole configurations related by reversal of the in-plane spi…

gr-qc2026

A stepping stone toward detecting gravitational wave memory: a cumulative analysis with the full spherical harmonic using events from GWTC-4.0 and GWTC-5.0

Maria Rosselló-Sastre, Sascha Husa, Yumeng Xu +3

We perform Bayesian model selection to test for the presence of the spherical harmonic mode in gravitational wave events that have previously been identified as bina…

astro-ph.HE2026

Remnant recoil and host environments of GWTC-4.0 binary black-hole mergers

Joan Llobera-Querol, Eleanor Hamilton, Neha Singh +8

Determining the astrophysical origin of binary black holes and whether merger remnants are retained in their birth environments is essential for understanding hierarchical mergers…

gr-qc2025

Hybrid waveforms for precessing quasi-circular binary systems

Joan Llobera-Querol, Sascha Husa, Maria de Lluc Planas

The demand for long and accurate gravitational waveforms is increasing as we prepare for the next generation of detectors and seek to improve current waveform models. However, nume…

gr-qc2024★ 5 cited

Building a bridge between comparable and extreme mass ratio black hole binaries: a single spin precessing model for the final state

Maria de Lluc Planas, Joan Llobera-Querol, Sascha Husa

Modelling the gravitational wave signal from binaries beyond comparable mass is an important open issue in gravitational wave astronomy. For non-spinning binaries and when the spin…