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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. 4.

Graphical representation of the Meyer cluster expansion. The coordinates are denoted by 1, 2, and 3 in the symbol for the three‐point function, while each vertex on the right‐hand side of the "equation" contains the possible tree and one‐loop connected components of the expansion. The lower left corner illustrates a disconnected term as an example, which is not used in our expansion.

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