Observational Constraints on High-Redshift Black Holes with JWST
Kavli Institute for Theoretical Physics via YouTube
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Explore observational constraints on high-redshift black holes with JWST in this 40-minute conference talk by Hannah Uebler from Cambridge. Recorded as part of the Cosmic Dawn Revealed by JWST conference at the Kavli Institute for Theoretical Physics, delve into the exciting exploration of cosmic dawn and the discoveries made possible by JWST. Gain insights into the nature of first stars, galaxies, and black hole seeds, as well as the stellar populations of early galaxies. Examine the star formation and chemical enrichment histories of these ancient cosmic structures. Investigate the key physical processes shaping the evolution of early galaxies and their black holes, and discover how near-field and deep field observations can be connected to form a comprehensive picture of the early universe.
Syllabus
Observational constraints on high-redshift black holes with JWST (R) â–¸ Hannah Uebler (Cambridge)
Taught by
Kavli Institute for Theoretical Physics