The Redshift Distribution of Distant Sources from Gravitational Depletion in Clusters

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dc.creatorMellier, Y.
dc.date1998-02-05
dc.date.accessioned2026-07-07T02:25:59Z
dc.date.available2026-07-07T02:25:59Z
dc.descriptionGravitational lensing can be used to analyze the redshift distribution of faint galaxies. In particular the magnification bias modifies locally the galaxy number density of lensed sources observed in lensing clusters. This depletion area probes the redshift distribution of galaxies beyond B=25. In this proceeding I present this new tool to infer the redhsift distribution of faint galaxies.
dc.descriptionTo appear in "The Young Universe". Ed. S. D'Odorico, A. Fontana & E. Giallongo, ASP Conf. Ser. Latex with paspconf.sty and psfig.sty. 4 pages, 2 figures. 43. Kb gzipped tar file
dc.identifierhttps://arxiv.org/abs/astro-ph/9802063
dc.identifierhttp://arxiv.org/abs/astro-ph/9802063
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12098
dc.subjectAstrophysics
dc.titleThe Redshift Distribution of Distant Sources from Gravitational Depletion in Clusters
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