Multiscale Methods

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dc.creatorSaar, E.
dc.date2006-12-14
dc.date.accessioned2026-07-07T07:34:26Z
dc.date.available2026-07-07T07:34:26Z
dc.descriptionThe lecture introduces a trous wavelet transforms, explains how to estimate the spatial density for galaxy distributions, and, finally, how to describe the morphology of cosmological density fields. An example application of these methods to the 2dFGRS gives unexpected results.
dc.description39 pages, 22 figures, to be published in the proceedings of the summer school "Data Analysis in Cosmology", Valencia, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0612370
dc.identifierhttp://arxiv.org/abs/astro-ph/0612370
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/119764
dc.subjectAstrophysics
dc.titleMultiscale Methods
dc.typetext

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