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.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.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.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 |