Mimicking the large-scale structure of the Local Universe - Synthetic pre-labelled galaxies in large-scale structures

Open Access

Table C.1.

Galaxy densities versus radial slices for cluster structures.

Shell	Inner	Outer	Galaxies	Volume	Density
	radius	radius
	Mpc	Mpc	%	[h⁻¹ Mpc]⁻³	${[\frac{galaxies}{(} h^{- 1} Mpc)}^{3}]$ $Mathematical equation: $ [\frac{\mathrm{galaxies}}(\mathrm{h}^{-1}\,\mathrm{Mpc})^{3}] $$
i	0.00	0.66	68.3	1.20	0.570n
ii	0.66	1.32	27.2	8.43	0.032n
iii	1.32	2.00	4.2	23.88	0.0017n

Total	0.00	2.00	99.7	33.51	0.0298n

Notes. n represents the number of galaxies within the cluster. In the example, n = Totalmassofcluster/Meangalaxymass = 10¹⁴ M_⊙/10¹¹ M_⊙ = 1000 [galaxies].

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.