Orateur
John Baker
(L2I Toulouse, CNRS/IN2P3, Université de Toulouse)
Description
As we prepare for LISA to open observations in the mHz gravitational wave observational band in the next decade, it is also time to begin considering what could come next? One goal for a future mHz-band observatory, or a network of observatories, would be to enhance the ability to localize sources. We discuss possible design strategies for architectures of future LISA-like missions to improve sky-localization, their relative capabilities for localizing mHz-band sources, and potential science opportunities for such missions.
| Which working group does your abstract concern? | Développement des détecteurs / Detectors development |
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Auteur
John Baker
(L2I Toulouse, CNRS/IN2P3, Université de Toulouse)