Speaker
Nikolaos Karnesis
(AUTh)
Description
LISA is going to be a signal-dominated observatory, thus, multiple Gravitational Wave signals from different types of sources are going to populate our future data streams. From those, the ones with high-enough SNR will be identified and subtracted from the data. However, we expect populations of sources that will generate a stochastic type of signal across the LISA band.
In this talk I will summarize the different possible contributions to the overall stochastic signal that we expect to measure with LISA, and also discuss the possible implications to data analysis.
Primary author
Nikolaos Karnesis
(AUTh)
