Study of the depletion effect in the cluster MS1008-1224

dc.creatorMayen, Christophe
dc.creatorSoucail, Genevieve
dc.date2000-06-14
dc.date.accessioned2026-07-07T01:53:58Z
dc.date.available2026-07-07T01:53:58Z
dc.descriptionWe present a detailed study of the depletion effect (the radial manifestation of the magnification bias) in the cluster MS1008-1224. Following our results concerning the simulations of depletion curves (see Mayen and Soucail, 2000 (astro-ph/0003332) for a complete description of the code), we propose to constrain the mass profile of the cluster and the main characteristics of its potential (orientation and ellipticity). This application is based solely on deep photometry of the field and does not require the measurement of the shape parameters of the faint background galaxies.
dc.description4 pages, includes 2 postscript figures, to appear in the proceedings of the XXth Moriond Astrophysics Meeting "Cosmological Physics with Gravitational Lensing", March 2000, eds. Y. Mellier, M. Mon, J. Tran Thanh Van, J.P. Kneib
dc.identifierhttps://arxiv.org/abs/astro-ph/0006197
dc.identifierhttp://arxiv.org/abs/astro-ph/0006197
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1165
dc.subjectAstrophysics
dc.titleStudy of the depletion effect in the cluster MS1008-1224
dc.typetext

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