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Fig. 2

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Spectral energy distribution of the GRB 980425 host (red), the WR region (blue), and the host with the WR region subtracted (green). The data are shown as squares and circles, whereas the Magphys and Grasil models are shown as solid and dotted lines, respectively. The empty blue circle denotes the ALMA flux of the WR region without the correction for the free-free emission. The mid-IR Spitzer/IRS spectrum of the WR region (Le Floc’h et al. 2012) is shown as a black line. The “host-WR” photometry almost overlaps with the total host photometry in most cases, so it is not shown. The data for the LMC are shown as black crosses (Israel et al. 2010; Meixner et al. 2013).

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