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Super massive black hole and host galaxy growth at the onset of strong feedback at z = 6 – 7.5

Published online by Cambridge University Press:  28 October 2024

Chiara Feruglio Open the ORCID record for Chiara Feruglio [Opens in a new window] ,
Manuela Bischetti ,
Roberta Tripodi ,
Fabrizio Fiore ,
Enrico Piconcelli  and
Luca Zappacosta
Chiara Feruglio*
Affiliation:
INAF - Osservatorio Astronomico di Trieste, Via G. Tiepolo 11, I-34143 Trieste, Italy
Manuela Bischetti
Affiliation:
Dipartimento di Fisica, Università di Trieste, Sezione di Astronomia, Via G.B. Tiepolo 11, I-34131 Trieste, Italy
Roberta Tripodi
Affiliation:
INAF - Osservatorio Astronomico di Trieste, Via G. Tiepolo 11, I-34143 Trieste, Italy Dipartimento di Fisica, Università di Trieste, Sezione di Astronomia, Via G.B. Tiepolo 11, I-34131 Trieste, Italy
Fabrizio Fiore
Affiliation:
INAF - Osservatorio Astronomico di Trieste, Via G. Tiepolo 11, I-34143 Trieste, Italy
Enrico Piconcelli
Affiliation:
INAF - Osservatorio Astronomico di Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy
Luca Zappacosta
Affiliation:
INAF - Osservatorio Astronomico di Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy
*
email: chiara.feruglio@inaf.it
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Abstract

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The first quasars at the Reionisation Epoch, z ∼ 6-7.5, probe the early stages of supermassive black holes and host galaxy assembly. In this paper, we present recent results, exploiting VLT, ALMA and NOEMA observations, that allow us to constrain the onset of strong black hole feedback, the dust properties and star formation rates in high redshift quasars with unprecedented accuracy. These results highlight the strategic importance of ALMA high frequency (i.e. Band 9 and 8) observations to obtain a reliable overview of the host galaxy and supermassive black hole growth out to the highest redshifts.

Keywords

QuasarsSupermassive black holesAGN host galaxiesBroad-absorption line quasarHigh-redshift galaxiesGalaxy evolution
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 19 , Symposium S378: Black Hole Winds at All Scales , December 2023 , pp. 76 - 83
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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