LOFAR/H-ATLAS: the low-frequency radio luminosity–star formation rate relation

LOFAR/H-ATLAS: the low-frequency radio luminosity–star formation rate relation

Radio emission is a key indicator of star formation activity in galaxies, but the radio luminosity–star formation relation has to date been studied almost exclusively at frequencies of 1.4 GHz or above. At lower radio frequencies, the effects of thermal radio emission are greatly reduced, and so we...

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Bibliografiska uppgifter
Huvudupphovsmän:	Gürkan, G, Hardcastle, M, Smith, D, Best, P, Bourne, N, Calistro-Rivera, G, Heald, G, Jarvis, M, Prandoni, I, Röttgering, H, Sabater, J, Shimwell, T, Tasse, C, Williams, W
Materialtyp:	Journal article
Publicerad:	Oxford University Press 2018

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