The SCUBA Half Degree Extragalactic Survey (SHADES) - IX : the environment, mass and redshift dependence of star formation
dc.contributor.author | Serjeant, S. | |
dc.contributor.author | Dye, S. | |
dc.contributor.author | Mortier, A. | |
dc.contributor.author | Peacock, J. | |
dc.contributor.author | Egami, E. | |
dc.contributor.author | Cirasuolo, M. | |
dc.contributor.author | Rieke, G. | |
dc.contributor.author | Borys, C. | |
dc.contributor.author | Chapman, S. | |
dc.contributor.author | Clements, D. | |
dc.contributor.author | Coppin, Kristen | |
dc.contributor.author | Dunlop, J. | |
dc.contributor.author | Eales, S. | |
dc.contributor.author | Farrah, D. | |
dc.contributor.author | Halpern, M. | |
dc.contributor.author | Mauskopf, P. | |
dc.contributor.author | Pope, A. | |
dc.contributor.author | Rowan-Robinson, M. | |
dc.contributor.author | Scott, D. | |
dc.contributor.author | Smail, I. | |
dc.contributor.author | Vaccari, M. | |
dc.date.accessioned | 2014-01-27T12:30:38Z | |
dc.date.available | 2014-01-27T12:30:38Z | |
dc.date.issued | 2008-06-01 | |
dc.identifier.citation | Serjeant , S , Dye , S , Mortier , A , Peacock , J , Egami , E , Cirasuolo , M , Rieke , G , Borys , C , Chapman , S , Clements , D , Coppin , K , Dunlop , J , Eales , S , Farrah , D , Halpern , M , Mauskopf , P , Pope , A , Rowan-Robinson , M , Scott , D , Smail , I & Vaccari , M 2008 , ' The SCUBA Half Degree Extragalactic Survey (SHADES) - IX : the environment, mass and redshift dependence of star formation ' , Monthly Notices of the Royal Astronomical Society , vol. 386 , no. 4 , pp. 1907-1921 . https://doi.org/10.1111/j.1365-2966.2008.13197.x | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | ORCID: /0000-0002-0729-2988/work/30423113 | |
dc.identifier.uri | http://hdl.handle.net/2299/12680 | |
dc.description | copyright Royal Astronomical Society | |
dc.description.abstract | We present a comparison between the SCUBA (Submillimetre Common User Bolometer Array) Half Degree Extragalactic Survey (SHADES) at 450 and 850 μm in the Lockman Hole East with a deep Spitzer Space Telescope survey at 3.6-24 μm conducted in guaranteed time. Using stacking analyses we demonstrate a striking correspondence between the galaxies contributing the submm extragalactic background light, with those likely to dominate the backgrounds at Spitzer wavelengths. Using a combination BRIzK plus Spitzer photometric redshifts, we show that at least a third of the Spitzer-identified submm galaxies at 1 <z <1.5 appear to reside in overdensities when the density field is smoothed at 0.5-2 Mpc comoving diameters, supporting the high-redshift reversal of the local star formation-galaxy density relation. We derive the dust-shrouded cosmic star formation history of galaxies as a function of assembled stellar masses. For model stellar masses | en |
dc.format.extent | 15 | |
dc.format.extent | 828243 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.title | The SCUBA Half Degree Extragalactic Survey (SHADES) - IX : the environment, mass and redshift dependence of star formation | en |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.description.status | Peer reviewed | |
dc.identifier.url | http://www.scopus.com/inward/record.url?scp=43749101316&partnerID=8YFLogxK | |
rioxxterms.versionofrecord | 10.1111/j.1365-2966.2008.13197.x | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true |