Probing the star formation epoch with Wilkinson Microwave Anisotropy Probe (WMAP) data and high-redshift QSOs

Details Probing the star formation epoch with Wilkinson Microwave Anisotropy Probe (WMAP) data and high-redshift QSOs Probing the star formation epoch with Wilkinson Microwave Anisotropy Probe (WMAP) data and high-redshift QSOs

2003-02-13

arxiv.org/abs/astro-ph/0302263v1

Publ.Astron.Soc.Jap. 55 (2003) L41

Astronomy and Astrophysics

Astrophysics

Scientific paper

Using the values of the cosmological parameters obtained from Wilkinson
Microwave Anisotropy Probe (WMAP) and the cosmological chemical clock observed
by high-redshift quasars, it is shown that star formation should have started
by the redshift $z_F > 9.5$, and that $z_F$ is sensitive only to $\omegamz h^2$
in flat $\Lambda$CDM cosmology.

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