Fig. 6.
Rest-frame SEDs of Herschel-SWIRE 500 μm sources with extreme starburst luminosities (SFR > 5000 M ⊙ yr−1), labelled with the redshift, whose optical through near-infrared SEDs are best-fitted by a QSO template. Alternative SWIRE associations are shown plotted below the extreme starburst solution. Possible redshift aliases (z comb)are shown plotted above the preferred z phot solution. Dotted loci: M 82 starburst, dashed loci: Arp 220 starburst, long-dashed loci: AGN dust torus. The constant C = 0 except in cases where SEDs are shown for both the photometric redshift and for a lower redshift alternative SWIRE association. In these cases C = −2 for the lower SED and +1 for the upper one.
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