dc.contributor.author | Takagi, T. | en_US |
dc.contributor.author | Mortier, A. M. J. | en_US |
dc.contributor.author | Shimasaku, K. | en_US |
dc.contributor.author | Coppin, K. | en_US |
dc.contributor.author | Pope, A. | en_US |
dc.contributor.author | Ivison, R. J. | en_US |
dc.contributor.author | Hanami, H. | en_US |
dc.contributor.author | Serjeant, S. | en_US |
dc.contributor.author | Clements, D. L. | en_US |
dc.contributor.author | Priddey, R. S. | en_US |
dc.contributor.author | Dunlop, J. S. | en_US |
dc.contributor.author | Takata, T. | en_US |
dc.contributor.author | Aretxaga, I. | en_US |
dc.contributor.author | Chapman, S. C. | en_US |
dc.contributor.author | Eales, S. A. | en_US |
dc.contributor.author | Farrah, D. | en_US |
dc.contributor.author | Granato, G. L. | en_US |
dc.contributor.author | Halpern, M. | en_US |
dc.contributor.author | Hughes, D. H. | en_US |
dc.contributor.author | van Kampen, E. | en_US |
dc.contributor.author | Scott, D. | en_US |
dc.contributor.author | Sekiguchi, K. | en_US |
dc.contributor.author | Smail, I. | en_US |
dc.contributor.author | Vaccari, M. | en_US |
dc.date.accessioned | 2014-03-12T19:20:59Z | |
dc.date.available | 2014-03-12T19:20:59Z | |
dc.date.issued | 2007-09-28 | en_US |
dc.identifier.citation | Takagi, T., A. M. J. Mortier, K. Shimasaku, K. Coppin, et al. 2007. "The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- V. Submillimetre properties of near-infrared--selected galaxies in the Subaru/XMM--Newton deep field." Monthly Notices of the Royal Astronomical Society 381(3): 1154-1168 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1111/j.1365-2966.2007.12302.x | en_US |
dc.identifier.uri | http://hdl.handle.net/10222/45447 | |
dc.description.abstract | We have studied the submillimetre (submm) properties of the following classes of near-infrared (NIR)-selected massive galaxies at high redshifts: BzK-selected star-forming galaxies (BzKs); distant red galaxies (DRGs); and extremely red objects (EROs). We used the SCUBA HAlf Degree Extragalactic Survey (SHADES), the largest uniform submm survey to date. Partial overlap of SIRIUS/NIR images and SHADES in SXDF has allowed us to identify 4 submm-bright NIR-selected galaxies, which are detected in the mid-infrared, 24 micron, and the radio, 1.4 GHz. We find that all of our submm-bright NIR-selected galaxies satisfy the BzK selection criteria, except for one galaxy whose B-z and z-K colours are however close to the BzK colour boundary. Two of the submm-bright NIR-selected galaxies satisfy all of the selection criteria we considered, i.e. they belong to the BzK-DRG-ERO overlapping population, or `extremely red' BzKs. Although these extremely red BzKs are rare (0.25 arcmin^{-2}), up to 20 % of this population could be submm galaxies. This fraction is significantly higher than that found for other galaxy populations studied here. Via a stacking analysis, we have detected the 850 micron flux of submm-faint BzKs and EROs in our SCUBA maps. While the contribution of z~2 BzKs to the submm background is about 10--15 % and similar to that from EROs typically at z~1, BzKs have a higher fraction (~30 %) of submm flux in resolved sources compared with EROs and submm sources as a whole. From the SED fitting analysis for both submm-bright and submm-faint BzKs, we found no clear signature that submm-bright BzKs are experiencing a specifically luminous evolutionary phase, compared with submm-faint BzKs. An alternative explanation might be that submm-bright BzKs are more massive than submm-faint ones. | en_US |
dc.title | The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- V. Submillimetre properties of near-infrared--selected galaxies in the Subaru/XMM--Newton deep field | en_US |
dc.title.alternative | Monthly Notices of the Royal Astronomical Society | en_US |
dc.type | article | en_US |
dc.identifier.volume | 381 | en_US |
dc.identifier.issue | 3 | en_US |
dc.identifier.startpage | 1154 | en_US |