Math 2.0

Astronomy and astrophysics Large-scale structure and physical cosmology Concept

Galaxy two-point correlation function

Summary

The galaxy two-point correlation function ξ(r)\xi(r) measures the excess probability, over a random distribution, of finding two galaxies at separation rr. It is the simplest statistic of galaxy clustering and the spatial analogue of an autocorrelation function. Its Fourier transform is the galaxy power spectrum, and on scales of a few megaparsecs it is close to a power law.

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Further reading

  1. Web https://en.wikipedia.org/wiki/Correlation_function_(astronomy)
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Changed3 November 2026

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