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Paper: Optical to FIR SED of Lyα Emitters
Volume: 446, Galaxy Evolution: Infrared to Millimeter Wavelength Perspective
Page: 383
Authors: Oteo, I.; Bongiovanni, A.; Pérez García, A. M.; Cepa, J.; Ederoclite, A.; Sánchez-Portal, M.; PEP team
Abstract: We present an optical and FIR analysis of a sample of 65 Lyα emitters at 2.0∼<z∼<3.5 selected from the final VIMOS spectroscopic campaign in the CDF-S (Popesso et al. 2009). For those objects, we fit the SED from 0.3 to 8.0 μm by using the GOODS-S MUSIC v.2. catalog (Santini et al. 2009.) and Bruzual & Charlot 2003 (BC03) templates, finding a continuous variety in their properties, more than a double nature, as previous works suggest. We find that five objects have PACS FIR counterparts and are (U)LIRGs candidates, being, therefore, dusty objects despite that they show Lyα in emission and with large equivalent widths.
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