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SUMMARY:Towards the LISA Global Fit - Christopher Moore (Cambridge)
DTSTART:20241024T150000Z
DTEND:20241024T160000Z
UID:TALK223345@talks.cam.ac.uk
CONTACT:Matthew Grayling
DESCRIPTION:The Laser Interferometer Space Antenna (LISA)\, one of ESA's u
 pcoming large-class missions\, is designed to detect gravitational waves (
 GWs) at millihertz frequencies. This frequency band containing an abundanc
 e of galactic\, extragalactic\, and cosmological sources. The large number
  of sources\, together with the fact that sources will be overlapping in b
 oth time and frequency\, requires the development of a new global approach
  to LISA data analysis where all the sources and instrument are characteri
 sed simultaneously. In this talk\, I will discuss the key data analysis ch
 allenges associated with the LISA global fit\, recent advances toward addr
 essing them\, and how these efforts align with LISA’s major scientific o
 bjectives.
LOCATION:Hoyle Lecture Theatre\, Institute of Astronomy
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