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Fig. 4.


Best-fitted SED for GRBH 061121. Red points are the observed fluxes with their uncertainties. The black line represents the best fitted spectrum composed of attenuated stellar emission, dust emission, non-thermal radio emission and nebular lines. The dashed blue line represents the unattenuated stellar emission and the blue shaded area indicates the amount dust attenuation. The lower panel shows the relative residual. The upper right panel is an enlargement of the UV/optical/NIR domain.

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