Learn how to use the time-domain simulation tools to generate a simple LDC-like dataset containing realistic instrumental noise and one MBHB signal. Learn how to quickly setup and run an MCMC on this dataset to estimate the source parameters.
Learn how to use the time-domain simulation tools to generate a simple LDC-like dataset containing realistic instrumental noise and one MBHB signal. Learn how to quickly setup and run an MCMC on this dataset to estimate the source parameters.
The parametrization of the instrumental noise and various effects (such as nonstationary noise, data artifacts, orbit faithfulness) will be demonstrated, as well as Galactic binary ensemble, and SGWB signals.
We will also show how to produce various TDI combinations, including Michelson XYZ and noise-orthogonal AET. This some of the expected noise-reduction steps.
A mini-global (band-limited) fit will be constructed, including first detection statistics followed by joint inference for some Galactic binaries, MHBHs, and instrument noise.
A mini-global (band-limited) fit will be constructed, including first detection statistics followed by joint inference for some Galactic binaries, MHBHs, and instrument noise.
