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Colloquium: A Good Hard Look at Growing Supermassive Black Holes in the Distant Universe

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Neil Brandt, Pennsylvania State University
When
16 October 2014 from 4:00 PM to 5:00 PM
Where
117 Osmond Laboratory
Contact Name
Eugenio Bianchi
Contact Phone
(814) 865-3147
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Sensitive cosmic X-ray surveys with the Chandra, XMM-Newton, and NuSTAR observatories have revolutionized our ability to find and study distant active galactic nuclei (AGNs), the main sites of supermassive black hole growth in the Universe. I will describe some of the resulting discoveries about the demographics, physics, and ecology of AGNs. Topics covered will include the utility of deep X-ray plus multiwavelength surveys for investigating distant AGNs; evolution constraints for the typical AGNs of the distant Universe; the cosmic balance of power between supermassive black holes and stars; interactions between AGNs and their hosting galaxies; and the AGN content of newly forming galaxies. I will end by discussing some key outstanding questions and new observations and missions that aim to answer them.

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