How galaxies populate haloes in very low-density environments - An analysis of the halo occupation distribution in cosmic voids

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Fig. A.2.

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HOD in MDPL2-SAG and TNG300 catalogues for the complete samples of voids (triangles) and voids with R_void > 13 h⁻¹ Mpc (circles). Left column: results for MDPL2-SAG and right column: TNG300. Top panels: limit magnitude M_r − 5 log₁₀(h) = − 18 and bottom panels: M_r − 5 log₁₀(h) = − 20. The uncertainties are calculated following the standard jackknife procedure.

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