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Fig. 10.

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Total GC numbers (NGC) for all the dwarf galaxies in this work. The vertical (grey) lines represent the NGC and their uncertainties for individual dwarf galaxies. The solid curve and the shaded regions around it represent the average (mean) NGC and 68% confidence intervals for dwarf galaxies within a moving bin along stellar mass (x-axis) with a width of 0.5 dex. The confidence intervals are based on 1000 bootstrap-repetitions of the estimates using bootstrap sample sizes of 95% of the initial sample sizes.

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