Euclid preparation - LXXXVIII. 3D reconstruction of the cosmic web with Euclid Deep spectroscopic samples

Open Access

Fig. B.3.

Multiplicity of central galaxies as a function of their stellar mass in Flagship (model m3) and GAEA (model ECLH) mocks, left and right panels, respectively, for M_*-limited samples ( $D_{M_{*}, noise, 60 %}$ $Mathematical equation: $ {\mathcal{D}}_{{M_{\ast}},\rm noise,\rm 60\%} $$ ), with M_*-weighted tessellation (qualitatively similar results are obtained without weighting).

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