Fig. 6
Optical-to-FIR observed SED of the PACS-detected Lymanα emitting galaxies. Blue dots represent the multi-wavelength photometry from U-band to MIPS-24 μm, and red dots are the PACS-100 μm and/or PACS-160 μm fluxes. The black curve represents the combination of BC03 and CE01 templates that best fit the photometric data for each galaxy.
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