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Fig. 3.


Normalised efficiency of LGRB hosts compared to the MOSDEF sample at 1 < z < 2 as a function of stellar mass (top left panel), SFR (top right panel), sSFR (bottom left panel) and metallicity (bottom right panel). The values are normalised to the first bin. The horizontal grey dashed line indicates a value of 1 to guide the eye.

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