Fig. 2.

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Mass fraction of stellar components. Upper panel: Mass fractions of the spheroidal component fsph as a function of galaxy stellar mass Mgal. Lower panel: Mass fractions of the discoidal component fdsk as a function of galaxy stellar mass Mgal. In both cases, the crosses with black solid line represent the original fsph or fdsk values for the nine equilibrium galaxies built using the AGAMA code (Vasiliev 2019) and the circles with a solid line show the fsph or fdsk values recovered with each of the six dynamical decomposition methods used.
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