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

Open Access

Table B.4.

Median and mean multiplicity for the GAEA ECLH and GAEA ECLQ mocks for tessellations with and without stellar mass weighting.


	GAEA ECLH				GAEA ECLQ

	median		mean		median		mean


	no weight	weight	no weight	weight	no weight	weight	no weight	weight

𝒟	2	2	1.69 ± 0.02	2.21 ± 0.01	2	2	1.61 ± 0.03	2.22 ± 0.02
𝒟^wFoG	1	2	1.36 ± 0.07	2.07 ± 0.04	1	2	1.28 ± 0.07	2.08 ± 0.04
𝒟^FoG, corr	2	2	1.61 ± 0.01	2.14 ± 0.01	2	2	1.62 ± 0.02	2.19 ± 0.02


𝒟_{M_*}	2	2	1.66 ± 0.01	1.78 ± 0.01	2	2	1.65 ± 0.01	1.80 ± 0.01
𝒟_{M_*}^wFoG	1	2	1.46 ± 0.04	1.78 ± 0.02	1	2	1.54 ± 0.04	1.79 ± 0.03
𝒟_{M_*}^FoG, corr	2	2	1.67 ± 0.01	1.80 ± 0.01	2	2	1.67 ± 0.01	1.85 ± 0.01


𝒟_60%	2	2	1.64 ± 0.07	2.17 ± 0.05	2	2	1.59 ± 0.11	2.15 ± 0.07
$D_{noise, 60 %}^{w FoG}$ $Mathematical equation: $ {\mathcal{D}}^{\mathrm{w FoG}}_{\mathrm{noise,60\%}} $$	1	2	1.50 ± 0.81	2.18 ± 0.33	1	2	1.28 ± 0.63	2.15 ± 0.46
$D_{M_{★}, noise, 60 %}^{FoG, corr}$ $Mathematical equation: $ {\mathcal{D}}^{\mathrm{FoG,corr}}_{M_\star,\rm noise,60\%} $$	1	2	1.49 ± 0.04	2.10 ± 0.05	1	2	1.47 ± 0.05	2.05 ± 0.06


$D_{M_{*}, 60 %}$ $Mathematical equation: $ {\mathcal{D}}_{{M_{\ast}},\rm 60\%} $$	2	2	1.60 ± 0.03	1.76 ± 0.02	2	2	1.60 ± 0.03	1.80 ± 0.03
$D_{M_{★}, noise, 60 %}^{w FoG}$ $Mathematical equation: $ {\mathcal{D}}^{\mathrm{w FoG}}_{M_\star,\rm noise,60\%} $$	1	2	1.43 ± 0.11	1.76 ± 0.08	1	2	1.50 ± 0.13	1.81 ± 0.09
$D_{M_{★}, noise, 60 %}^{FoG, corr}$ $Mathematical equation: $ {\mathcal{D}}^{\mathrm{FoG,corr}}_{M_\star,\rm noise,60\%} $$	2	2	1.63 ± 0.03	1.77 ± 0.03	2	2	1.62 ± 0.04	1.81 ± 0.04

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