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Fig. 3

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Evolution of the halo and disc masses, and their characteristic scales for 411321 TVP. Green, red, and blue lines with dots show the parameters recovered from the IllustrisTNG-100 data. Solid black lines correspond to the values after the interpolation and smoothing with a time step of 1 Myr, which was used in the orbital integration. The dashed lines represent the 5 Gyr duration.

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