Evidence for dark energy: cross-correlating SDSS5 and WMAP3

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dc.creatorA, Cabre.
dc.creatorE, Gaztanaga.
dc.creatorM, Manera.
dc.creatorP, Fosalba.
dc.creatorF, Castander.
dc.date2006-11-02
dc.date.accessioned2026-07-07T07:30:38Z
dc.date.available2026-07-07T07:30:38Z
dc.descriptionWe cross-correlate the third-year WMAP data with galaxy samples extracted from the SDSS DR5 (SDSS5) covering 16% of the sky. These measurements confirm a positive cross-correlation, which is well fitted by the integrated Sachs-Wolfe (ISW) effect for flat LCDM models with a cosmological constant.
dc.descriptionProceeding for the Cosmic Frontiers 06 conference in Durham
dc.identifierhttps://arxiv.org/abs/astro-ph/0611046
dc.identifierhttp://arxiv.org/abs/astro-ph/0611046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118470
dc.subjectAstrophysics
dc.titleEvidence for dark energy: cross-correlating SDSS5 and WMAP3
dc.typetext

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