Four GRB afterglows are modeled from radio to X-rays, all favoring a wind-like external medium, with the shock magnetic field declining as t^{-3/4}.
The observations at 9.0 GHz resulted in four detections and one upper limit
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The GROND GRB sample: II. Fireball parameters for four GRB afterglows
Four GRB afterglows are modeled from radio to X-rays, all favoring a wind-like external medium, with the shock magnetic field declining as t^{-3/4}.