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Fig. 3.

image

Separating stellar and gas-phase components at the GRB explosion site. Top: original spectrum (black) extracted from the spaxel nearest to the GRB position and fitted stellar component (red). Second: zoom-in of the continuum. Third: resulting spectrum of the gas-phase contribution (blue). Bottom: zoom-in of the gas-phase contribution (blue) together with the error spectrum (black).

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