Speaker
Stefan Strub
Description
The Laser Interferometer Space Antenna (LISA) is aimed to measure gravitational waves in the mili-Hertz frequency band, which is dominated by millions of Galactic binaries. While some of these binaries produce signals that are extractable, most of them blur into a confusion foreground. We introduce a new approach to extract the best-fitting solutions for Galactic binaries across the entire frequency band from data with multiple overlapping signals. Furthermore, we use these best-fitting solutions to omit the burn-in stage and to take full advantage of GPU-accelerated signal simulation, allowing us to compute posterior distributions in just 2.3 seconds per signal on a laptop-grade GPU.
Author
Stefan Strub
Co-authors
Dr
Cedric Schmelzbach
(ETH Zurich)
Dr
Luigi Ferraioli
(ETH Zurich)
Dr
Simon Stähler
(ETH Zurich)
Prof.
Domenico Giardini
(ETH Zurich)