Fig. 4
Left panel: SFR map in the galaxy for the two fields covered by PMAS observations, computed using the Kennicutt (1989) diagnostic. Right panel: specific SFR obtained by weighting the SFR map and the rest-frame B-luminosity map, applying the same method described in Christensen et al. (2004). The dimensions of each spaxel have been interpolated in the figure, showing elements of 0.25 × 0.25 arcsec. The SLSN position is marked with a white cross.
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