Studies of galaxy clustering through the use of binary tree hierarchies. I - Multipoint correlation functions

Statistics – Computation

Scientific paper

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Computational Astrophysics, Galactic Clusters, Astronomical Catalogs, Correlation Coefficients

Scientific paper

The study presents a method for evaluating multipoint correlation functions using the analysis of the structure of a 'binary tree' which spans the particular set of galaxies under consideration. A recursive center-of-mass transformation is used and a binary tree data structure is compiled. For a large number of particles, N, the computational expense for constructing the tree increases as N log N. The M-point correlation functions are also determined by recursively scanning the nodes of the tree and binning the m-tuplets discovered by the scan. Gains of more than two orders of magnitude in computational speed are attained for that possible by direct counting of m-tuplets. This permits the examination of much larger data sets or of higher-order correlation than has been possible thus far.

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