Figures and Tables

From the following article:

Simulations of the formation, evolution and clustering of galaxies and quasars

Volker Springel, Simon D. M. White, Adrian Jenkins, Carlos S. Frenk, Naoki Yoshida, Liang Gao, Julio Navarro, Robert Thacker, Darren Croton, John Helly, John A. Peacock, Shaun Cole, Peter Thomas, Hugh Couchman, August Evrard, Jörg Colberg & Frazer Pearce

Nature 435, 629-636(2 June 2005)

doi:10.1038/nature03597

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Figure 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 1

The dark matter density field on various scales.

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Figure 2

Differential halo number density as a function of mass and epoch.

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Figure 3

Environment of a 'first quasar candidate' at high and low redshifts.

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Figure 4

Galaxy two-point correlation function, xi(r), at the present epoch as a function of separation r.

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Figure 5

Galaxy clustering as a function of luminosity and colour.

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Figure 6

Power spectra of the dark matter and galaxy distributions in the baryon oscillation region.

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