The Swift/Fermi GRB 080928 from 1 eV to 150 keV | Astronomy & Astrophysics (A&A)

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Fig. 11

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The SED of galaxy G1 close to the afterglow (see Fig. 10), obtained from images taken with GROND 6.5 months after the burst (g′r′i′z′JHK_s filters). Shown is the best HyperZ fit that is based on the template of a dusty starburst galaxy at a redshift of z = 1.46 (see also Table 7).

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