activity
20192021
most citedComputationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes

581 citations · 1.8k across the 10 of their papers we have counts for

collaborators

10 papers

gr-qc2021★ 79 cited

A detailed analysis of GW190521 with phenomenological waveform models

Héctor Estellés, Sascha Husa, Marta Colleoni +8

In this paper we present an extensive analysis of the GW190521 gravitational wave event with the current (fourth) generation of phenomenological waveform models for binary black ho…

gr-qc2021★ 117 cited

New twists in compact binary waveform modelling: a fast time domain model for precession

Héctor Estellés, Marta Colleoni, Cecilio García-Quirós +5

We present IMRPhenomTPHM, a phenomenological model for the gravitational wave signals emitted by the coalescence of quasi-circular precessing binary black holes systems. The model…

gr-qc2021★ 16 cited

Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1

Maite Mateu-Lucena, Sascha Husa, Marta Colleoni +5

We consider the ten confidently detected gravitational-wave signals in the GWTC-1 catalog which are consistent with mergers of binary black hole systems, and perform a thorough par…

gr-qc2020★ 5 cited

Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Héctor Estellés, Sascha Husa, Marta Colleoni +5

In this work we present an extension of the time domain phenomenological model IMRPhenomT for gravitational wave signals from binary black hole coalescences to include subdominant…

gr-qc2020★ 44 cited

Towards the routine use of subdominant harmonics in gravitational-wave inference: re-analysis of GW190412 with generation X waveform models

Marta Colleoni, Maite Mateu-Lucena, Héctor Estellés +5

We re-analyse the gravitational-wave event GW190412 with state-of-the-art phenomenological waveform models. This event, which has been associated with a black hole merger, is inter…

astro-ph.IM2020★ 503 cited

Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue

I. M. Romero-Shaw, C. Talbot, S. Biscoveanu +56

Gravitational waves provide a unique tool for observational astronomy. While the first LIGO--Virgo catalogue of gravitational-wave transients (GWTC-1) contains eleven signals from…

gr-qc2020★ 581 cited

Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes

Geraint Pratten, Cecilio García-Quirós, Marta Colleoni +8

We present IMRPhenomXPHM, a phenomenological frequency-domain model for the gravitational-wave signal emitted by quasi-circular precessing binary black holes, which incorporates mu…

gr-qc2020★ 43 cited

Accelerating the evaluation of inspiral-merger-ringdown waveforms with adapted grids

Cecilio García-Quirós, Sascha Husa, Maite Mateu-Lucena +1

This paper presents an algorithm to accelerate the evaluation of inspiral-merger-ringdown waveform models for gravitational wave data analysis. While the idea can also be applied i…

gr-qc2020★ 323 cited

IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries

Cecilio García-Quirós, Marta Colleoni, Sascha Husa +5

We present the IMRPhenomXHM frequency domain phenomenological waveform model for the inspiral, merger and ringdown of quasi-circular non-precessing black hole binaries. The model e…

gr-qc2019★ 72 cited

A first survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation

Antoni Ramos-Buades, Sascha Husa, Geraint Pratten +5

We analyze a new numerical relativity dataset of spinning but nonprecessing binary black holes on eccentric orbits, with eccentricities from approximately to , with dime…