The nature of the faint sub-mJy radio population
| dc.creator | Seymour, Nick | |
| dc.creator | McHardy, Ian | |
| dc.creator | Gunn, Katherine | |
| dc.creator | Moss, Derek | |
| dc.date | 2004-11-01 | |
| dc.date.accessioned | 2026-07-07T02:15:37Z | |
| dc.date.available | 2026-07-07T02:15:37Z | |
| dc.description | The up-turn in Euclidean normalised source counts below 1mJy at 1.4GHz is well established in many deep radio surveys. There are strong reasons, observationally and theoretically, to believe that this up-turn is due to strong evolution of the starforming population up to z=2. However this hypothesis needs further confirmation spectroscopically and the examples in the literature are sparse. Theoretically the up-turn is well modelled by the evolution of the local radio starforming population and is consistent with the up-turn seen in recent mid-infrared source counts at 15um (ISOCAM) and 24um (Spitzer) and the tight correlation of the radio and MIR Luminosities of starforming galaxies. | |
| dc.description | 2 Pages, including 2 PostScript figures. To appear in the proceedings of "The Dusty and Molecular Universe. A prelude to HERSCHEL and ALMA" 27 - 29 October 2004, Paris | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0411015 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0411015 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8471 | |
| dc.subject | Astrophysics | |
| dc.title | The nature of the faint sub-mJy radio population | |
| dc.type | text |