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Tugwell, L. Marchetti, L. Vigroux, L. Wang, M. Griffin, M. J. Page, M. Pohlen, M. Rowan-Robinson, M. Symeonidis, M. Vaccari, M. Viero, N. Seymour, O. Ilbert, P. Chanial, R. Auld, S. Eales, S. Heinis, S. J. Oliver, V. Buat","submitted_at":"2011-05-03T18:03:51Z","abstract_excerpt":"As part of the Herschel Multi-tiered Extragalactic Survey we have investigated the rest-frame far-infrared (FIR) properties of a sample of more than 4800 Lyman Break Galaxies (LBGs) in the Great Observatories Origins Deep Survey North field. Most LBGs are not detected individually, but we do detect a sub-sample of 12 objects at 0.7 < z < 1.6 and one object at z ~ 2.0.\n  The ones detected by Herschel SPIRE have redder observed NUV-U and U-R colors than the others, while the undetected ones have colors consistent with average LBGs at z > 2.5. 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