Fig. 7
Observations of the host galaxy of GRB 090205 shown with data points and upper limits are compared with synthetic SEDs for a starburst galaxy with different stellar ages τ. From top to bottom, lines corresponds to τ = 500, 100, 50, 10 Myr, respectively. We assume a Salpeter IMF between 0.1–100 M⊙, Z = 0.4Z⊙ and no dust extinction in the host galaxy. The SED are normalized to reproduce the observation in the I band.
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