Introduction

• Quentin Baghi (APC | Université Paris Cité)
• Jean-Baptiste Bayle (University of Glasgow)
• Eleonora Castelli (NASA GSFC | UMBC)
• Natalia Korsakova (APC)

Getting Started (1/2)

• Jean-Baptiste Bayle (University of Glasgow)
• Quentin Baghi (APC | Université Paris Cité)
• Maude Le Jeune (APC)

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.

Getting Started (2/2)

• Maude Le Jeune (APC)
• Quentin Baghi (APC | Université Paris Cité)
• Jean-Baptiste Bayle (University of Glasgow)

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.

Simulation in depth

• Martin Staab (SYRTE)
• Quentin Baghi (APC | Université Paris Cité)
• Henri Inchauspé (Institute for Theoretical Physics, Universität Heidelberg)
• Christian Chapman-Bird (University of Glasgow)
• Eleonora Castelli (NASA GSFC | UMBC)
• Jean-Baptiste Bayle (University of Glasgow)
• Olaf Hartwig
• Maude Le Jeune (APC)

The parametrization of the instrumental noise and various effects (such as nonstationary noise, data artifacts, orbit faithfulness) will be demonstrated, as well as realistic time-domain EMRI, 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.

Towards a global fit (1/2)

• Maude Le Jeune (APC)
• Sylvain Marsat (L2I Toulouse, CNRS/IN2P3, UT3)
• Quentin Baghi (APC | Université Paris Cité)
• Natalia Korsakova (APC)
• Nikolaos Karnesis (AUTh)
• Senwen Deng (APC)
• Michael Katz (NASA Marshall)

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.

Towards a global fit (2/2)

• Natalia Korsakova (APC)
• Quentin Baghi (APC | Université Paris Cité)
• Sylvain Marsat (L2I Toulouse, CNRS/IN2P3, UT3)
• Maude Le Jeune (APC)
• Nikolaos Karnesis (AUTh)
• Senwen Deng (APC)
• Michael Katz (NASA Marshall)

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.