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Nastasi, Alessandro (2012): Multiwavelength Study of high redshift galaxy clusters. Dissertation, LMU München: Fakultät für Physik

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Figure 2.1: Energy density curves of the three main components of the universe(matter, radiation and dark energy) as a function of redshift and for different cosmo-logical models
Figure 2.2: The Cosmic Microwave Background as seen by COBE (top) and WMAP
Figure 2.3: The time evolution of the dark matter power spectrum in the MillenniumSimulation
Figure 2.4: Differential dark matter halo number density as a function of mass and
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