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Fig. 1.

image

Galaxy-wide IMFs computed using IGIMF3 as a function of stellar mass plotted for several values of SFR (10−3 – blue, 1.0 – green, 103 – red M yr−1) and [Fe/H] (−3, 0 2). The galaxy-wide IMFs are normalised by their values at 1 M to show the slope changes. The universal K01 IMF is plotted as a black dashed line.

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