Speaker
Dr
Riccardo Buscicchio
(Universitá di Milano-Bicocca, Milan, IT)
Description
In this talk, we explore two assumptions ubiquitous in LISA data analysis: Gaussianity and stationarity of astrophysical noise sources (i.e. arising from source confusion). I will provide an overview on characterizations and parameter estimations techniques of both properties. I will review the most recent findings on the Galactic population of double white dwarfs and the extragalactic one of extreme mass-ratio inspirals. Employing a suite of advanced statistical techniques, we aim to enhance our understanding of the noise properties and improve the overall data modeling process.
| Contribution length | Middle |
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Authors
Federico Pozzoli
(University of Insubria, Como, IT)
Manuel Piarulli
(L2IT, Université Toulouse III - Paul Sabatier)
Dr
Riccardo Buscicchio
(Universitá di Milano-Bicocca, Milan, IT)
