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Fig. A.1

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Well-behaved assembly histories for all mass components of the halo identified as FoFID 28000000000013. We plot M200c as a solid black line with crosses, M* as a solid salmon line with “×”-shaped markers, and MBH as a solid red line with small diamonds. The corresponding curve fit functions are shown as dashed lines with coloured dots (blue for M200c, yellow for M*, and light grey for MBH). The horizontal black dashed lines represent t50% and t70%. We observe that these histories display discrete behaviour with some degree of discontinuity. Using methods like curve fitting could result in significantly different estimates for the half-mass assembly time, which we aim to avoid. This example demonstrates that the interpolation approach, without any fit, provides a more accurate result.

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