Fig. 3 from A Simulation of Galaxy Formation and Clustering

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A Simulation of Galaxy Formation and Clustering

Authors: F. R. Pearce, A. Jenkins, C. S. Frenk, J. M. Colberg, S. D. M. White, P. A. Thomas, H. M. P. Couchman, J. A. Peacock, G. Efstathiou, and The Virgo Consortium

Pearce et al. 1999 The Astrophysical Journal Letters 521 L99.

Provider: AAS Journals

Caption: Fig. 3.

Mass and galaxy correlation functions. The dashed lines show the mass correlation functions at ﹩z=3﹩ and ﹩z=0﹩. The solid, long‐dashed, and dotted lines show the galaxy correlation functions in the simulation at the indicated redshifts. The squares show the observed, real‐space correlation function, estimated by Baugh (1996), from the APM survey.

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