The Open UniversitySkip to content
 

LOFAR-Boötes: Properties of high- and low-excitation radio galaxies at 0.5 < z < 2.0

Williams, W. L.; Calistro Rivera, G.; Best, P. N.; Hardcastle, M. J.; Röttgering, H. J. A.; Duncan, K. J.; de Gasperin, F.; Jarvis, M. J.; Miley, G. K.; Mahony, E. K.; Morabito, L. K.; Nisbet, D. M.; Prandoni, I.; Smith, D. J. B.; Tasse, C. and White, G. J. (2018). LOFAR-Boötes: Properties of high- and low-excitation radio galaxies at 0.5 < z < 2.0. Monthly Notices of the Royal Astronomical Society (In Press).

Google Scholar: Look up in Google Scholar

Abstract

This paper presents a study of the redshift evolution of radio-loud active galactic nuclei (AGN) as a function of the properties of their galaxy hosts in the Boötes field. To achieve this we match low-frequency radio sources from deep 150-MHz LOFAR observations to an I-band-selected catalogue of galaxies, for which we have derived photometric redshifts, stellar masses and rest-frame colours. We present spectral energy distribution (SED) fitting to determine the mid-infrared AGN contribution for the radio sources and use this information to classify them as High- versus Low-Excitation Radio Galaxies (HERGs and LERGs) or Star-Forming galaxies. Based on these classifications we construct luminosity functions for the separate redshift ranges going out to z = 2. From the matched radio-optical catalogues, we select a sub-sample of 624 high power (P150MHz > 1025 W Hz-1) radio sources between 0.5 ≤ z < 2. For this sample, we study the fraction of galaxies hosting HERGs and LERGs as a function of stellar mass and host galaxy colour. The fraction of HERGs increases with redshift, as does the fraction of sources in galaxies with lower stellar masses. We find that the fraction of galaxies that host LERGs is a strong function of stellar mass as it is in the local Universe. This, combined with the strong negative evolution of the LERG luminosity functions over this redshift range, is consistent with LERGs being fuelled by hot gas in quiescent galaxies.

Item Type: Journal Item
Copyright Holders: 2016 The Authors
ISSN: 1365-2966
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 52622
Depositing User: G. J. White
Date Deposited: 13 Dec 2017 11:15
Last Modified: 19 Dec 2017 10:07
URI: http://oro.open.ac.uk/id/eprint/52622
Share this page:

Actions (login may be required)

Policies | Disclaimer

© The Open University   contact the OU