Supermassive black holes at high redshifts

Journal
Date Issued
2019
Author(s)
Ajello, Marco
•
Paliya, Vaidehi
•
Marcotulli, Lea
•
Perkins, Jeremy S.
•
•
•
DE ANGELIS, ALESSANDRO
•
Thompson, David
•
•
Dominguez, Alberto
•
Beckmann, Volker
•
Guiriec, Sylvain
•
Wadiasingh, Zorawar
•
Coppi, Paolo
•
Harding, J. Patrick
•
Petropoulou, Maria
•
Hewitt, John W.
•
Ojha, Roopesh
•
Marcowith, Alexandre
•
•
Castro, Daniel
•
Baring, Matthew
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Hays, Elizabeth
•
•
Bozhilov, Vladimir
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Tomsick, John
•
Agudo, Ivan
•
Venters, Tonia
•
McEnery, Julie
•
The, Lih-Sin
•
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
Uri
Url
Issn Identifier
2330-9458
Ads BibCode
2019BAAS...51c.289A
Rights
open.access
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