Black hole and galaxy co-evolution in radio-loud active galactic nuclei at z ~ 0.3–4

Poitevineau, R.; Castignani, G.; Combes, F.

doi:10.1051/0004-6361/202244560

Black hole and galaxy co-evolution in radio-loud active galactic nuclei at z ~ 0.3–4

Journal Article · Wed Apr 19 00:00:00 EDT 2023 · Astronomy and Astrophysics

DOI:https://doi.org/10.1051/0004-6361/202244560· OSTI ID:2423193

Poitevineau, R. ^[1]; Castignani, G. ^[2]; Combes, F. ^[3]

Paris Observatory (France); Paris Sciences et Lettres University (France); Centre National de la Recherche Scientifique (CNRS) (France); Sorbonne Univ., Paris (France)
Univ. of Bologna (Italy); Istituto Nazionale di Astrofisica (INAF) (Italy)
College de France, Paris (France)

The relation between the mass of the supermassive black hole (SMBH) in the center of galaxies and their bulge mass or central velocity dispersion is well known. This suggests a coevolution between the SMBHs and their galaxy hosts. Our aim is to study this relation, specifically, for radio loud galaxies, and as a function of redshift z. We selected a sample of 42 radio galaxies and active galactic nuclei (AGN) with broad emission lines and spectroscopic redshifts between z = 0.3 - 4 by cross-matching the low radio frequency sources from Very Large Array (VLA) FIRST with spectroscopically confirmed galaxies from wide-field surveys, including Sloan Digital Sky Survey (SDSS) DR14 ugriz and Dark Energy Survey (DES) DR2 grzY in the optical, Wield Infrared Survey Explorer (WISE), and the Galaxy And Mass Assembly (GAMA) spectroscopic survey. We characterized the stellar mass (M_$$\star$$), star formation, and black hole properties (mass of the central SMBH, Eddington ratio η, and jet power, Q_jet). The relation between SMBH mass, M_$$\star$$, η, and z is placed into context by comparing them with scaling relations (M_BH–M_$$\star$$, M_BH/M_$$\star$$–z, M_BH–Q_jet, and Q_jet–η) from the literature. On the basis of a multiwavelength spectral energy distribution modeling, our radio sources are broadly consistent with being on the star-forming main sequence. They have sub-Eddington accretion rates, η ≃ 1% on average, as typically found in type I AGN, while higher accretion rates favor more powerful jets to be launched by the central engine. We find overmassive SMBHs in (17 ± 5)% of our radio sources, similarly to previous studies on nearby early-type galaxies. Altogether, an evolutionary scenario in which radio-mode AGN feedback regulates the accretion onto the SMBHs and the stellar mass assembly of the radio sources is discussed, which may explain the observed phenomenology. This pilot study represents a benchmark for future studies using wide-field surveys such as those with Euclid and the Vera Rubin Observatory.

View Accepted Manuscript (DOE)

Research Organization:: Argonne National Laboratory (ANL), Argonne, IL (United States)

Sponsoring Organization:: USDOE

Grant/Contract Number:: AC02-06CH11357

OSTI ID:: 2423193

Journal Information:: Astronomy and Astrophysics, Journal Name: Astronomy and Astrophysics Vol. 672; ISSN 0004-6361

Publisher:: EDP SciencesCopyright Statement

Country of Publication:: United States

Language:: English

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The X–shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars Farina, Emanuele Paolo; Schindler, Jan-Torge; Walter, Fabian The Astrophysical Journal, Vol. 941, Issue 2 https://doi.org/10.3847/1538-4357/ac9626	journal	December 2022
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First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter The Astrophysical Journal, Vol. 875, Issue 1 https://doi.org/10.3847/2041-8213/ab0ec7	journal	April 2019
First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter The Astrophysical Journal Letters, Vol. 930, Issue 2 https://doi.org/10.3847/2041-8213/ac6674	journal	May 2022
On the Connection between Supermassive Black Holes and Galaxy Growth in the Reionization Epoch Li, Junyao; Silverman, John D.; Izumi, Takuma The Astrophysical Journal Letters, Vol. 931, Issue 1 https://doi.org/10.3847/2041-8213/ac6de8	journal	May 2022

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79 ASTRONOMY AND ASTROPHYSICS
galactic bulge
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Black hole and galaxy co-evolution in radio-loud active galactic nuclei at z ~ 0.3–4

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