Cosmic Magnification

dc.creatorMenard, Brice
dc.date2002-10-07
dc.date.accessioned2026-07-07T02:05:35Z
dc.date.available2026-07-07T02:05:35Z
dc.descriptionI present the current status of the cosmic magnification produced by systematic amplification of background sources by large-scale structures. After introducing its principle, I focus on its interests for cosmology and underline its complementary aspect to cosmic shear and galaxy auto-correlations. I finally discuss recent investigations using higher-order statistics.
dc.description4 pages, 1 figure, Proceedings SF2A-2002, Paris, ed. F. Combes and D. Barret, EDP-Sciences
dc.identifierhttps://arxiv.org/abs/astro-ph/0210142
dc.identifierhttp://arxiv.org/abs/astro-ph/0210142
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5147
dc.subjectAstrophysics
dc.titleCosmic Magnification
dc.typetext

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