Cosmic Shear and Clusters of Galaxies

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dc.creatorMellier, Y.
dc.creatorvan Waerbeke, L.
dc.creatorErben, T.
dc.creatorSchneider, P.
dc.creatorBernardeau, F.
dc.creatorJain, B.
dc.creatorMaoli, R.
dc.creatorFort, B.
dc.creatorDantel-Fort, M.
dc.creatorCuillandre, J. -C.
dc.creatorCracken, H. Mc
dc.creatorFevre, O. Le
dc.date2000-09-30
dc.date.accessioned2026-07-07T01:55:44Z
dc.date.available2026-07-07T01:55:44Z
dc.descriptionThe first detections of cosmic shear signal reported recently by 4 independent groups cover angular scales between one and 10 arcmin. On those scales, the cosmic shear is a signature of non-linear perturbations, like groups and clusters of galaxies. We present the results obtained by our team on CFHT and on the VLT and discuss its impact for the analysis of cluster abundances and cosmology
dc.descriptionLatex, 7 pages, iap2000.sty and psfig.sty, gzipped tar file. To appear in the Proceedings of the IAP2000 conference "Constructing the Universe with Clusters of Galaxies", eds. D. Gerbal, F. Durret
dc.identifierhttps://arxiv.org/abs/astro-ph/0010008
dc.identifierhttp://arxiv.org/abs/astro-ph/0010008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1759
dc.subjectAstrophysics
dc.titleCosmic Shear and Clusters of Galaxies
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