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Observational Constraints on Higher Order Clustering up to z ≃ 1

  • Authors: István Szapudi, Marc Postman, Tod R. Lauer, and William Oegerle

Szapudi et al. 2001 The Astrophysical Journal 548 114.

  • Provider: AAS Journals

Caption: Fig. 3.

Constraints on the time evolution of biasing. The shaded band shows the predicted ﹩s_{3}﹩ from a simple model (see § 5 for details). Filled symbols show ﹩S_{3}﹩ measured at 0﹩\fdg﹩04, where the FORCE error bars are the smallest. Strictly, each ﹩S_{3}﹩ is at a slightly different scale in comoving ﹩h^{-1}\,\mathrm{Mpc}\,﹩, but because of the flat scaling of ﹩S_{3}﹩ this is not an important effect. The centered error bars on all data points are those derived from the FORCE package. The right‐shifted error bars for the two faintest data points are the ﹩\mathrm{FORCE}\,+\mathrm{systematic}\,﹩ errors (see § 4.1.1 for details).

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