Orateur
Natalia Korsakova
(APC)
Description
LISA is a signal-dominated instrument that will observe thousands of sources, from binaries in our galaxy to massive black hole binaries at very high redshift. However, the same aspect that makes LISA data so rich also makes it difficult to analyse. I will discuss the challenges that LISA data analysis poses and the ways we can overcome them. In particular, I will focus on two aspects: the global fit, including how we approach parameter estimation for galactic binaries and its difficulties; and low-latency parameter estimation for massive black hole binaries, which is important for electromagnetic follow-ups.
