HerMES: Lyman break galaxies individually detected at 0.7 ≤ z ≤ 2.0 in goods-N with Herschel/spire
- Burgarella, D.
- Heinis, S.
- Magdis, G.
- Auld, R.
- Blain, A.
- Bock, J.
- Brisbin, D.
- Buat, V.
- Chanial, P.
- Clements, D.
- Cooray, A.
- Eales, S.
- Franceschini, A.
- Giovannoli, E.
- Glenn, J.
- Gonzlez Solares, E.
- Griffin, M.
- Hwang, H.
- Ilbert, O.
- Marchetti, L.
- Mortier, A.
- Oliver, S.
- Page, M.
- Papageorgiou, A.
- Pearson, C.
- Pérez-Fournon, I.
- Pohlen, M.
- Rawlings, J.
- Raymond, G.
- Rigopoulou, D.
- Rodighiero, G.
- Roseboom, I.
- Rowan-Robinson, M.
- Scott, D.
- Seymour, Nick
- Smith, A.
- Symeonidis, M.
- Tugwell, K.
- Vaccari, M.
- Vieira, J.
- Viero, M.
- Vigroux, L.
- Wang, L.
- Wright, G.
DOIAbstract
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 2.5. The UV-to-FIR spectral energy distributions of the objects detected in the rest-frame FIR are investigated using the code CIGALE to estimate physical parameters. We find that LBGs detected by SPIRE are high-mass, luminous infrared galaxies. It appears that LBGs are located in a triangle-shaped region in the A FUV versus log L FUV = 0 diagram limited by A FUV = 0 at the bottom and by a diagonal following the...
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