| dc.contributor.author | Serjeant, S. | en_US |
| dc.contributor.author | Negrello, M. | en_US |
| dc.contributor.author | Pearson, C. | en_US |
| dc.contributor.author | Mortier, A. | en_US |
| dc.contributor.author | Austermann, J. | en_US |
| dc.contributor.author | Aretxaga, I. | en_US |
| dc.contributor.author | Clements, D. | en_US |
| dc.contributor.author | Chapman, S. | en_US |
| dc.contributor.author | Dye, S. | en_US |
| dc.contributor.author | Dunlop, J. | en_US |
| dc.contributor.author | Dunne, L. | en_US |
| dc.contributor.author | Farrah, D. | en_US |
| dc.contributor.author | Hughes, D. | en_US |
| dc.contributor.author | Lee, H. -M | en_US |
| dc.contributor.author | Matsuhara, H. | en_US |
| dc.contributor.author | Ibar, E. | en_US |
| dc.contributor.author | Im, M. | en_US |
| dc.contributor.author | Jeong, W. -S | en_US |
| dc.contributor.author | Kim, S. | en_US |
| dc.contributor.author | Oyabu, S. | en_US |
| dc.contributor.author | Takagi, T. | en_US |
| dc.contributor.author | Wada, T. | en_US |
| dc.contributor.author | Wilson, G. | en_US |
| dc.contributor.author | Vaccari, M. | en_US |
| dc.contributor.author | Yun, M. | en_US |
| dc.date.accessioned | 2014-03-12T19:20:59Z | |
| dc.date.available | 2014-03-12T19:20:59Z | |
| dc.date.issued | 2010-02-18 | en_US |
| dc.identifier.citation | Serjeant, S., M. Negrello, C. Pearson, A. Mortier, et al. 2010. "The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light." Astronomy and Astrophysics 514:10. | en_US |
| dc.identifier.issn | 0004-6361 | |
| dc.identifier.uri | http://hdl.handle.net/10222/45428 | |
| dc.identifier.uri | http://dx.doi.org/10.1051/0004-6361/200913483 | |
| dc.description.abstract | We present a comparison of the SCUBA Half Degree Extragalactic Survey (SHADES) at 450, 850 and 1100 microns with deep guaranteed time 15 microns AKARI FU-HYU survey data and Spitzer guaranteed time data at 3.6-24 microns in the Lockman Hole East. The AKARI data was analysed using bespoke software based in part on the drizzling and minimum-variance matched filtering developed for SHADES, and was cross calibrated against Infrared Space Observatory (ISO) fluxes. Our stacking analyses find AKARI 15um galaxies with >~200 microJy contribute >10% of the 450 micron background, but only 0.3. | en_US |
| dc.relation.isformatof | Astronomy and Astrophysics | |
| dc.title | The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light | en_US |
| dc.title.alternative | arXiv:1002.3618 [astro-ph] | en_US |
| dc.type | article | en_US |
| dc.identifier.issue | 514 | |
| dc.identifier.startpage | 10 | en_US |
