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SUMMARY:Beyond Gauss? A more accurate model for LISA astrophysical noise s
 ource - Riccardo Buscicchio (University of Milano-Bicocca)
DTSTART:20241015T130000Z
DTEND:20241015T140000Z
UID:TALK222178@talks.cam.ac.uk
CONTACT:Steven Brereton
DESCRIPTION:In this talk\, I explore two assumptions ubiquitous in LISA da
 ta analysis: Gaussianity and stationarity of astrophysical noise sources (
 i.e. arising from source confusion). I will provide an overview on detecti
 on and parameter estimations techniques for both properties. I will review
  the most recent findings on the Galactic population of double white dwarf
 s and the extragalactic one of extreme mass-ratio inspirals. Employing a s
 uite of advanced statistical techniques\, we aim to enhance our understand
 ing of the noise properties and improve the overall data modeling process\
 , a core element of any global fit.
LOCATION:Hoyle Lecture Theatre\, Institute of Astronomy
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