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Glitch systematics on the observation of massive black-hole binaries with LISA
Alice Spadaro, Riccardo Buscicchio, Daniele Vetrugno +6
Detecting and coherently characterizing thousands of gravitational-wave signals is a core data-analysis challenge for the Laser Interferometer Space Antenna (LISA). Transient artif…
On the LISA science performance in observations of short-lived signals from massive black hole binary coalescences
Geraint Pratten, Antoine Klein, Christopher J. Moore +4
The observation of massive black hole binary systems is one of the main science objectives of the Laser Interferometer Space Antenna (LISA). The instrument's design requirements ha…
EFPE: Efficient fully precessing eccentric gravitational waveforms for binaries with long inspirals
Antoine Klein
In this paper, we derive a set of equations of motions for binaries on eccentric orbits undergoing spin-induced precession that can efficiently be integrated on the radiation-react…
Prospects for Fundamental Physics with LISA
Enrico Barausse, Emanuele Berti, Thomas Hertog +318
In this paper, which is of programmatic rather than quantitative nature, we aim to further delineate and sharpen the future potential of the LISA mission in the area of fundamental…
Convergence of Fourier-domain templates for inspiraling eccentric compact binaries
Sashwat Tanay, Antoine Klein, Emanuele Berti +1
The space-based detector LISA may observe gravitational waves from the early inspiral of stellar-mass black hole binaries, some of which could have significant eccentricity. Curren…
Post-Newtonian phase accuracy requirements for stellar black hole binaries with LISA
Alberto Mangiagli, Antoine Klein, Alberto Sesana +2
The Laser Interferometer Space Antenna (LISA) will observe black hole binaries of stellar origin during their gravitational wave inspiral, months to years before coalescence. Due t…