by Marco Ajello, Vaidehi Paliya, Lea Marcotulli, Jeremy S. Perkins, Elisa Prandini, Filippo D'Ammando, Alessandro De Angelis, David Thompson, Hui Li, Alberto Dominguez, Volker Beckmann, Sylvain Guiriec, Zorawar Wadiasingh, Paolo Coppi, J. Patrick Harding, Maria Petropoulou, John W. Hewitt, Roopesh Ojha, Alexandre Marcowith, Michele Doro, Daniel Castro, Matthew Baring, Elizabeth Hays, Elena Orlando, Sylvain Guiriec, Vladimir Bozhilov, John Tomsick, Ivan Agudo, Tonia Venters, Julie McEnery, Lih-Sin The, Dieter Hartmann, Sara Buson, Francesco Longo, and Dario Gasparrini
Published onMay 31, 2019
Supermassive black holes at high redshifts
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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.
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