The evolution of the low-frequency radio AGN population to z 1.5 in the ELAIS N1 field
Loading...
Date
2020-11-13
Authors
Journal Title
Journal ISSN
Volume Title
Publisher
Advance Access publication
Abstract
We study the cosmic evolution of radio sources out to z 1.5 using a GMRT 610 MHz survey covering ∼1.86 deg2 of the ELAIS
N1 field with a minimum/median rms noise 7.1/19.5 μJy beam−1 and an angular resolution of 6 arcsec. We classify sources
as star forming galaxies (SFGs), radio-quiet (RQ) and radio-loud (RL) Active Galactic Nuclei (AGNs) using a combination
of multiwavelength diagnostics and find evidence in support of the radio emission in SFGs and RQ AGN arising from star
formation, rather than AGN-related processes. At high luminosities, however, both SFGs and RQ AGN display a radio excess
when comparing radio and infrared star formation rates. The vast majority of our sample lie along the SFR − M ‘main
sequence’ at all redshifts when using infrared star formation rates. We derive the 610 MHz radio luminosity function for the
total AGN population, constraining its evolution via continuous models of pure density and pure luminosity evolution with
∝ ( 1 + z)
(2.25±0.38)−(0.63±0.35)z and L610 MHz ∝ ( 1 + z)
(3.45±0.53)−(0.55±0.29)z
, respectively. For our RQ and RL AGN, we find
a fairly mild evolution with redshift best fitted by pure luminosity evolution with L610 MHz ∝ ( 1 + z)
(2.81±0.43)−(0.57±0.30)z for
RQ AGN and L610 MHz ∝ ( 1 + z)
(3.58±0.54)−(0.56±0.29)z for RL AGN. The 610 MHz radio AGN population thus comprises two
differently evolving populations whose radio emission is mostly SF-driven or AGN-driven, respectively.
Description
Keywords
galaxies, luminosity function, large-scale structure of Universe, radio continuum
Citation
Ocran et al. 2021.The evolution of the low-frequency radio AGN population to z ≃ 1.5 in the ELAIS N1 field, Monthly Notices of the Royal Astronomical Society,500(4):4685–4702,