New twists in compact binary waveform modeling: A fast time-domain model for precession
H. Estellés(Universitat de les Illes Balears), A. Ramos-Buades(Max Planck Institute for Gravitational Physics), Maria de Lluc Planas(Universitat de les Illes Balears), M. Mateu-Lucena(Universitat de les Illes Balears), C. García-Quirós(Universitat de les Illes Balears), S. Husa(Maastricht University), D. Keitel(University of Washington Bothell), M. Colleoni(Fundació Universitat-Empresa de les Illes Balears)
Cited by 104
Related Papers
Frequency-domain gravitational waves from nonprecessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
|Physical review. D/Physical review. D.|2016|800
Computationally efficient models for the dominant and subdominant harmonic modes of precessing binary black holes
|Physical review. D/Physical review. D.|2021|543
Bayesian inference for compact binary coalescences with <scp>bilby</scp>: validation and application to the first LIGO–Virgo gravitational-wave transient catalogue
|Monthly Notices of the Royal Astronomical Society|2020|468
Multimode frequency-domain model for the gravitational wave signal from nonprecessing black-hole binaries
|Physical review. D/Physical review. D.|2020|308
Setting the cornerstone for a family of models for gravitational waves from compact binaries: The dominant harmonic for nonprecessing quasicircular black holes
|Physical review. D/Physical review. D.|2020|279