Beyond Gauss? A more accurate model for LISA astrophysical noise source

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• Riccardo Buscicchio (University of Milano-Bicocca)
• Tuesday 15 October 2024, 14:00-15:00
• Hoyle Lecture Theatre, Institute of Astronomy.

If you have a question about this talk, please contact Steven Brereton.

KICC Special Seminar

In this talk, I 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 detection and parameter estimations techniques for 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, a core element of any global fit.

This talk is part of the Kavli Institute for Cosmology Seminars series.

This talk is included in these lists:

• Cambridge Astronomy Talks
• Combined External Astrophysics Talks DAMTP
• Cosmology, Astrophysics and General Relativity
• Hoyle Lecture Theatre, Institute of Astronomy
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists

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