Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-03-14
Publ.Astron.Soc.Austral. 22 (2005) 136
Astronomy and Astrophysics
Astrophysics
12 pages, 6 figures, accepted for publication in PASA
Scientific paper
10.1071/AS05006
Filaments of galaxies are the dominant feature of modern large scale redshift surveys. They can account for up to perhaps half of the baryonic mass budget of the Universe and their distribution and abundance can help constrain cosmological models. However, there remains no single, definitive way in which to detect, describe and define what filaments are and their extent. This work examines a number of physically motivated, as well as statistical, methods that can be used to define filaments and examines their relative merits.
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