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1
Intro
2
LISA and the Global Fit
3
Outline GW parameter estimation for LISA
4
Laser Interferometer Space Antenna (LISA)
5
LISA sources
6
LISA Data Challenges
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LDC Radler (challenge 1)
8
What is Gibbs Sampling?
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Why Gibbs Sampling?
10
Global Fit Design
11
Catalog production
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Catalog results
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Catalog usage Developer's view
14
Corner case 1 Developer's view
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Corner case 2 Developer's view
Description:
Explore the global analysis of galactic binary gravitational wave signals in this 27-minute conference talk by Kristen Lackeos from the Max Planck Institute for Radio Astronomy. Delve into the challenges and techniques of extracting overlapping galactic signals using the Laser Interferometer Space Antenna (LISA). Learn about the 'GBMCMC' pipeline for global fitting of Galactic white dwarf binaries and its application to simulated data from LISA Data Challenges. Discover the post-analysis and science of resulting catalog data, methods to quantify pipeline search efficacy, and future developments towards global fitting of multiple gravitational wave source types. Gain insights into LISA's capabilities, the dominance of ultra-compact binary signals in the milli-Hertz frequency band, and the complexities of resolving individual sources from the galactic foreground.

LISA and the Global Analysis of Galactic Binary Gravitational Wave Signals

Institute for Pure & Applied Mathematics (IPAM)
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