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arXiv · 1609.07527

High-Redshift AGNs and the Next Decade of Chandra and XMM-Newton

W. N. Brandt·F. Vito
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Abstract

We briefly review how X-ray observations of high-redshift active galactic nuclei (AGNs) at z = 4-7 have played a critical role in understanding their basic demographics as well as their physical processes; e.g., absorption by nuclear material and winds, accretion rates, and jet emission. We point out some key remaining areas of uncertainty, highlighting where further Chandra and XMM-Newton observations/analyses, combined with new multiwavelength survey data, can advance understanding over the next decade.

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W. N. Brandt, F. Vito. 2016-11-08. High-Redshift AGNs and the Next Decade of Chandra and XMM-Newton. https://doi.org/10.1002/asna.201713337

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