Supermassive black holes at high redshifts
Date Issued
2019
Author(s)
Ajello, Marco
•
Paliya, Vaidehi
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Marcotulli, Lea
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Perkins, Jeremy S.
•
•
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DE ANGELIS, ALESSANDRO
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Thompson, David
•
•
Dominguez, Alberto
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Beckmann, Volker
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Guiriec, Sylvain
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Wadiasingh, Zorawar
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Coppi, Paolo
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Harding, J. Patrick
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Petropoulou, Maria
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Hewitt, John W.
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Ojha, Roopesh
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Marcowith, Alexandre
•
•
Castro, Daniel
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Baring, Matthew
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Hays, Elizabeth
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Bozhilov, Vladimir
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Tomsick, John
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Agudo, Ivan
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Venters, Tonia
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McEnery, Julie
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The, Lih-Sin
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Hartmann, Dieter
•
Buson, Sara
•
Longo, Francesco
•
Abstract
MeV blazars are the most luminous sources in the Universe and host supermassive black holes. An MeV survey will detect >1000 of them up to z > 5. This would allow us: to probe the formation and growth of massive black holes at high z; to pinpoint the emission region location in blazars; to determine the interplay of accretion and black hole spin.
Volume
51
Issue
3
Start page
289
Issn Identifier
2330-9458
Ads BibCode
2019BAAS...51c.289A
Rights
open.access
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