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Fig. 5


Spectral energy distribution of HAE229 (black filled circles). We show the template SED (solid line) of a main-sequence galaxy at z = 2 (Magdis et al. 2012) which is based on models (Draine & Li 2007). In addition, template SEDs of observed SMGs are shown for comparison: ALESS SMG composite (dotted line – Swinbank et al. 2014), average SED of 73 spectroscopically identified SMGs (dashed line – Michałowski et al. 2010), and an average SED of SMGs (dashed-dotted line – Pope et al. 2008). The far-infrared SED is matched by the different SMG composites whereas the rest-frame optical SED shows that HAE229 is redder than the average of various types of dusty vigorously star-forming galaxies at high redshift.

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