Whittam, I. H. and Jarvis, M. J. and Hale, C. L. and Prescott, M. and Morabito, L. K. and Heywood, I. and Adams, N. J. and Afonso, J. and An, Fangxia and Ao, Y. and Bowler, R. A. and Collier, J. D. and Deane, R. P. and Delhaize, J. and Frank, B. and Glowacki, M. and Hatfield, P. W. and Maddox, N. and Marchetti, L. and Matthews, A. M. and Prandoni, I. and Randriamampandry, S. and Randriamanakoto, Z. and Smith, D. J. B. and Taylor, A. R. and Thomas, N. L. and Vaccari, M. (2022) 'MIGHTEE: the nature of the radio-loud AGN population.', Monthly notices of the Royal Astronomical Society., 516 (1). pp. 245-263.
We study the nature of the faint radio source population detected in the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Early Science data in the COSMOS field, focusing on the properties of the radio-loud active galactic nuclei (AGNs). Using the extensive multiwavelength data available in the field, we are able to classify 88 per cent of the 5223 radio sources in the field with host galaxy identifications as AGNs (35 per cent) or star-forming galaxies (54 per cent). We select a sample of radio-loud AGNs with redshifts out to z ∼ 6 and radio luminosities 1020 < L1.4 GHz/W Hz−1 < 1027 and classify them as high-excitation and low-excitation radio galaxies (HERGs and LERGs). The classification catalogue is released with this work. We find no significant difference in the host galaxy properties of the HERGs and LERGs in our sample. In contrast to previous work, we find that the HERGs and LERGs have very similar Eddington-scaled accretion rates; in particular we identify a population of very slowly accreting AGNs that are formally classified as HERGs at these low radio luminosities, where separating into HERGs and LERGs possibly becomes redundant. We investigate how black hole mass affects jet power, and find that a black hole mass ≳ 107.8 M⊙ is required to power a jet with mechanical power greater than the radiative luminosity of the AGN (Lmech/Lbol > 1). We discuss that both a high black hole mass and black hole spin may be necessary to launch and sustain a dominant radio jet.
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|Publisher Web site:||https://doi.org/10.1093/mnras/stac2140|
|Publisher statement:||© The Author(s) 2022. Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.|
|Date accepted:||24 July 2022|
|Date deposited:||06 September 2022|
|Date of first online publication:||24 August 2022|
|Date first made open access:||06 September 2022|
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