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Fig. 6.

image

Stellar mass content in central and satellite galaxies for MDPL2-SAG (left) and TNG300 (right) catalogues. Upper panels: ⟨M|Mhalo⟩ as a function of the halo mass for galaxies inside voids (triangles) and all galaxies (squares). Bottom panels: ratio between M for galaxies in voids and the overall population. Dashed lines correspond to central galaxies and dotted lines to the satellite population. Error bars are computed using the standard jackknife procedure.

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