Fig. A.2

NIR through to X-ray SEDs of the 32 GRBs analysed that did not enter our final sample. Frequency is plotted in the rest-frame and flux density is in arbitrary units for clarity. The SEDs have been corrected for Galactic reddening and soft X-ray absorption, and both the host galaxy absorbed/extinguished (solid) and intrinsic (dashed) best-fit afterglow SED are indicated. The afterglow SEDs are ordered by afterglow host galaxy extinction, with the most extinguished at the bottom, and the least at the top.
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