Measures of the galaxy clustering

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dc.creatorMartinez, Vicent J.
dc.date1996-03-13
dc.date.accessioned2026-07-07T02:20:59Z
dc.date.available2026-07-07T02:20:59Z
dc.descriptionA brief introduction is given to some aspects of the statistical description of the luminous matter distribution. I review the features of the redshift surveys that arise in the statistical analysis of the galaxy clustering. Special topics include intensity functions, correlation functions, correlation integrals, multifractals and multiscaling.
dc.description10 pages, uuencoded, gzipped LaTeX file using ioplppt.sty (enclosed) 29 kByte, 5 figures (not enclosed, hard copies of figures available upon request from: martinez@hubble.matapl.uv.es). Proc. ``International School of Physics Enrico Fermi'', Course CXXXII: Dark Matter in the Universe, Varenna 1995, eds.: S. Bonometto, J. Primack, A. Provenzale, IOP, to appear
dc.identifierhttps://arxiv.org/abs/astro-ph/9603054
dc.identifierhttp://arxiv.org/abs/astro-ph/9603054
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10400
dc.subjectAstrophysics
dc.titleMeasures of the galaxy clustering
dc.typetext

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