Orateurs
Sylvain Marsat
(L2I Toulouse, CNRS/IN2P3)
Stanislav Babak
(APC)
Description
This tutorial shows the general process to follow when analyzing LDC data to detect and characterize gravitational-waves from massive black hole binary sources.
The objective is to:
1. Load and plot the TDI data in time and frequency domain
2. Compute a source SNR
3. Compute a likelihood
4. Transformation to LISA frame and how it helps
6. Perform parameter estimation in the noiseless case
