AEGIS20: a radio survey of the Extended Groth Strip
| dc.contributor.author | Ivison, R. J. | en_US |
| dc.contributor.author | Chapman, S. C. | en_US |
| dc.contributor.author | Faber, S. M. | en_US |
| dc.contributor.author | Smail, Ian | en_US |
| dc.contributor.author | Biggs, A. D. | en_US |
| dc.contributor.author | Conselice, C. J. | en_US |
| dc.contributor.author | Wilson, G. | en_US |
| dc.contributor.author | Salim, S. | en_US |
| dc.contributor.author | Huang, J. -S | en_US |
| dc.contributor.author | Wilner, S. P. | en_US |
| dc.date.accessioned | 2014-03-12T19:20:54Z | |
| dc.date.available | 2014-03-12T19:20:54Z | |
| dc.date.issued | 2007-05-01 | en_US |
| dc.description.abstract | We describe AEGIS20 - a radio survey of the Extended Groth Strip (EGS) conducted with the Very Large Array (VLA) at 1.4GHz. The resulting catalog contains 1,123 emitters and is sensitive to ultraluminous starbursts to z1 where correcting for contamination by radio-loud active galactic nuclei (AGN) comes at the price of rejecting luminous starbursts. Whilst stacking radio images is a useful technique, accurate radio-based SFRs for z>>1 galaxies require precise redshifts and extraordinarily high-fidelity radio data to identify and remove accretion-related emission. | en_US |
| dc.identifier.citation | Ivison, R. J., S. C. Chapman, S. M. Faber, Ian Smail, et al. 2007. "AEGIS20: a radio survey of the Extended Groth Strip." The Astrophysical Journal 660(1): 77-L80 | en_US |
| dc.identifier.issn | 0004-637X | en_US |
| dc.identifier.issue | 1 | en_US |
| dc.identifier.startpage | 77 | en_US |
| dc.identifier.uri | http://dx.doi.org/10.1086/517917 | en_US |
| dc.identifier.uri | http://hdl.handle.net/10222/45349 | |
| dc.identifier.volume | 660 | en_US |
| dc.title | AEGIS20: a radio survey of the Extended Groth Strip | en_US |
| dc.title.alternative | The Astrophysical Journal | en_US |
| dc.type | article | en_US |
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