Galaxy and mass assembly (GAMA): the 325 MHz radio luminosity function of AGN and star-forming galaxies

Measurement of the evolution of both active galactic nuclei (AGN) and star-formation in galaxies underpins our understanding of galaxy evolution over cosmic time. Radio continuum observations can provide key information on these two processes, in particular via the mechanical feedback produced by ra...

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Bibliographic Details
Main Authors:	Prescott, M, Mauch, T, Jarvis, M, McAlpine, K, Smith, D, Fine, S, Johnston, R, Hardcastle, M, Baldry, I, Brough, S, Brown, M, Bremer, M, Driver, S, Hopkins, A, Kelvin, L, Loveday, J, Norberg, P, Obreschkow, D, Sadler, E
Format:	Journal article
Published:	Oxford University Press 2016

Galaxy and mass assembly (GAMA): the 325 MHz radio luminosity function of AGN and star-forming galaxies

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