FIR Measurements of Lyα Emitters at z <~ 1.0: Dust Attenuation from PACS-Herschel
One remaining open question regarding the physical properties of Lyα emitters (LAEs) is their dust content and evolution with redshift. The variety of results is large and with those reported by now it is difficult to establish clear relations between dust, other fundamental parameters of galaxies (star formation rate, metallicity, or age), and
Oteo, I. et al.
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2011