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Test for LISA foreground Gaussianity and stationarity: Extreme mass-ratio inspirals

Manuel Piarulli ^1,2,*, Riccardo Buscicchio ^2,3,†, Federico Pozzoli ⁴, Ollie Burke ¹, Matteo Bonetti ², and Alberto Sesana ²

¹Laboratoire des 2 Infinis-Toulouse (L2IT-IN2P3), Université de Toulouse, CNRS, UPS, F-31062 Toulouse Cedex 9, France
²Dipartimento di Fisica “G. Occhialini,” Universitá degli Studi di Milano-Bicocca and INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, 20126 Milano, Italy
³Institute for Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham, Birmingham, B15 2TT, United Kingdom
⁴Dipartimento di Scienza e Alta Tecnologia, Universitá degli Studi dell’Insubria, I-22100 Como, Italy

^*Contact author: manuel.piarulli@l2it.in2p3.fr
^†Contact author: riccardo.buscicchio@unimib.it

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Articles Citing

Test for LISA foreground Gaussianity and stationarity: Extreme mass-ratio inspirals

Evolution of ultracompact neutron star–helium star binaries

Angular resolution of a Bayesian search for anisotropic stochastic gravitational wave backgrounds with LISA

Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries

Prototype stochastic gravitational wave background recovery in the LISA global fit residual

Efficient waveforms for asymmetric-mass eccentric equatorial inspirals into rapidly spinning black holes

Test for LISA foreground Gaussianity and stationarity: galactic white-dwarf binaries

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