Large-scale distribution of galaxies - Filamentary structure and visual bias

Statistics – Computation

Scientific paper

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Computational Astrophysics, Cosmology, Galactic Clusters, Pattern Recognition, Red Shift, Sky Surveys (Astronomy), Spatial Distribution, Statistical Analysis, Visual Perception

Scientific paper

It is shown that the eye is good at detecting global coherence and at the same time easily fooled into seeing large-scale filamentary features where none exists. For this reason an objective method of identification that also assesses statistical significance is necessary to confirm or reject the presence of filaments in the distribution of galaxies. It has been found that a construction called the minimal spanning tree (MST), together with a data-permuting technique, works very well. The validity of this procedure is demonstrated on Glass patterns, and it is shown that the subjective interpretation of visual cues must be questioned. The MST procedure applied to the CfA redshift data finds statistical evidence for the presence of filamentary features.

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