Open Access

Table 1.

Cosmological and structure formation parameters used to obtain the CSFR.

Ω0, m Ω0, b Ω0, Λ h zi σ8 np Mmin(M)
0.279 0.0463 0.721 0.7 20 0.84 0.967 106

Notes. Ω0, m corresponds to the total matter (baryonic plus DM) density parameter; Ω0, b is the baryonic density parameter; Ω0, Λ is the density parameter associated with dark energy (cosmological constant); h is the Hubble constant written as H0 = 100 h km s−1 Mpc−1; zi is the redshift at which star formation begins; σ8 is the normalization of the power spectrum, in other words σ(M, 0); np is the spectral index of the power spectrum; Mmin corresponds to the lowest mass a DM halo must have to detach from the expansion of the Universe, to collapse, and to virialize (it is approximately equal to the Jeans mass at recombination).

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.