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Fig. 1.

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Distribution of the percentage difference between the stellar masses from Subfind and 2 × R M star / 2 r op $ 2 \times R_{M_{\mathrm {star}}/2}\sim r_{\mathrm {op}} $ apertures under different constrains. The black, red, and blue lines correspond to measurements within halocentric radius R500c, R200c, and the mass considered by the FoF algorithm, respectively. The dashed lines represent the normal distribution fitted to each constraint and are shown in their corresponding colour.

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