Lecture

Gravitational Waves and the Hubble Constant

Description

This lecture discusses the measurement of the Hubble Constant using gravitational waves, focusing on the standard siren method. It explores how the Hubble Constant posterior is estimated, the impact of electromagnetic counterparts, and the importance of galaxy catalogues. The presentation showcases the analysis of binary black hole mergers and binary neutron star mergers, emphasizing the role of Bayesian modeling and galaxy redshift estimation.

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