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Fig. 1.

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Stellar mass of the complete sample of low-mass galaxies available in the Auriga Project as a function of their M200 mass at z = 0. In this work, we only analyse those galaxies that have more than 10 000 stellar particles, which translates into M* ≥ 6 × 107M. The horizontal dashed line represents this threshold in stellar mass in logarithmic scale. The galaxies used in this work are colour-coded by their amount of accreted stellar mass.

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