The faint radio source population at 15.7 GHz – IV. The dominance of core emission in faint radio galaxies

dc.contributor.author	Whittam, I. H.
dc.contributor.author	Green, D. A.
dc.contributor.author	Jarvis, M. J.
dc.date.accessioned	2021-02-10T11:04:52Z
dc.date.available	2021-02-10T11:04:52Z
dc.date.issued	2020
dc.identifier.citation	Whittam, I. H. et al. (2020). The faint radio source population at 15.7 GHz – IV. The dominance of core emission in faint radio galaxies. Monthly Notices of the Royal Astronomical Society, 493(2), 2841–2853	en_US
dc.identifier.issn	1365-2966
dc.identifier.uri	https://doi.org/10.1093/mnras/staa306
dc.identifier.uri	http://hdl.handle.net/10566/5887
dc.description.abstract	We present 15-GHz Karl G. Jansky Very Large Array observations of a complete sample of radio galaxies selected at 15.7 GHz from the Tenth Cambridge (10C) survey. 67 out of the 95 sources (71 per cent) are unresolved in the new observations and lower frequency radio observations, placing an upper limit on their angular size of ∼2 arcsec.	en_US
dc.language.iso	es	en_US
dc.publisher	Oxford University Press	en_US
dc.subject	Catalogues	en_US
dc.subject	Galaxies: active	en_US
dc.subject	Radio continuum: galaxies	en_US
dc.subject	Surveys	en_US
dc.title	The faint radio source population at 15.7 GHz – IV. The dominance of core emission in faint radio galaxies	en_US
dc.type	Article	en_US