Fig. 9
Spectral energy distributions at two different time intervals. The SED for IBIS and Fermi/LAT data from T0 + 300 s to T0 + 1050 s (light-grey stars), and the SED for GROND and Swift/XRT at T0 + 26 ks (black circles). The IBIS and Fermi/LAT data are also shown rescaled (dark-grey stars) to the GROND-Swift/XRT SED to illustrate the single-spectra component from X-rays to GeV.
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