The LoTSS view of radio AGN in the local Universe

• Published in: Astronomy and astrophysics (Berlin) 2019-02, Vol.622
• Main Authors: Sabater, J., Best, P. N., Hardcastle, M. J., Shimwell, T. W., Tasse, C., Williams, W. L., Brüggen, M., Cochrane, R. K., Croston, J. H., de Gasperin, F., Duncan, K. J., Gürkan, G., Mechev, A. P., Morabito, L. K., Prandoni, I., Röttgering, H. J. A., Smith, D. J. B., Harwood, J. J., Mingo, B., Mooney, S., Saxena, A.
• Format: Article
• Language: English
• Subjects: Active galactic nuclei; Dependence; Galaxies; galaxies: active; galaxies: evolution; LOFAR; Luminosity; Radio astronomy; radio continuum: galaxies; Radio emission; Radio sources (astronomy); Sky surveys (astronomy); Star & galaxy formation; Star formation; Stellar mass; Stellar mass accretion; surveys; Universe
• ISSN: 0004-6361; 1432-0746
• DOI: 10.1051/0004-6361/201833883

This paper presents a study of the local radio source population, by cross-comparing the data from the first data release (DR1) of the LOFAR Two-Metre Sky Survey (LoTSS) with the Sloan Digital Sky Survey (SDSS) DR7 main galaxy spectroscopic sample. The LoTSS DR1 provides deep data (median rms noise of 71 μJy at 150 MHz) over 424 square degrees of sky, which is sufficient to detect 10 615 (32 per cent) of the SDSS galaxies over this sky area. An improved method to separate active galactic nuclei (AGN) accurately from sources with radio emission powered by star formation (SF) is developed and applied, leading to a sample of 2121 local (z  1011 M⊙) displaying radio-AGN activity with L150 MHz ≥ 1021 W Hz−1; thus, the most massive galaxies are always switched on at some level. The results allow the full Eddington-scaled accretion rate distribution (a proxy for the duty cycle) to be probed for massive galaxies, and this accretion rate is found to peak at Lmech/LEdd ≈ 10−5. More than 50 per cent of the energy is released during the ≤2 per cent of the time spent at the highest accretion rates, Lmech/LEdd > 10−2.5. Stellar mass is shown to be a more important driver of radio-AGN activity than black hole mass, suggesting a possible connection between the fuelling gas and the surrounding halo. This result is in line with models in which these radio AGN are essential for maintaining the quenched state of galaxies at the centres of hot gas haloes.