Fig. 4.

VLT/MUSE view of the host of GRB 050709: E(B − V) in units of magnitudes. Grid coordinates are given in units of arcseconds relative to the emission-line object Q shown in Fig. 1. The circles have the same meaning as in Fig. 1. The “AG” refers to the region that includes the afterglow position. One spaxel () corresponds to 0.57 × 0.57 kpc2. We note that the positional accuracy of these regions on the MUSE images compared to the HST image is about ±1 spaxel.
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