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Fig. A.1.
Metallicity of the LGRB host galaxies of the BAT6 sample at 1 < z < 2 versus the peak of the ν Fν (left panel) and the isotropic-equivalent luminosity (right panel) of the prompt emission of the corresponding LGRB (from Pescalli et al. 2016). The points are colour-coded by redshift. The arrows indicate lower limits.
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