Takagi, T.Mortier, A. M. J.Shimasaku, K.Coppin, K.Pope, A.Ivison, R. J.Hanami, H.Serjeant, S.Clements, D. L.Priddey, R. S.Dunlop, J. S.Takata, T.Aretxaga, I.Chapman, S. C.Eales, S. A.Farrah, D.Granato, G. L.Halpern, M.Hughes, D. H.van Kampen, E.Scott, D.Sekiguchi, K.Smail, I.Vaccari, M.2014-03-122014-03-122007-09-28Takagi, 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): 1154-11680035-8711http://dx.doi.org/10.1111/j.1365-2966.2007.12302.xhttp://hdl.handle.net/10222/45447We 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.article38131154