A combined HST/CFH12k/XMM survey of X-ray luminous clusters of galaxies at z~0.2

Simple item page
dc.creatorCzoske, Oliver
dc.creatorKneib, Jean-Paul
dc.creatorSmail, Ian
dc.creatorSmith, Graham P.
dc.creatorEbeling, Harald
dc.date2000-07-11
dc.date.accessioned2026-07-07T01:54:20Z
dc.date.available2026-07-07T01:54:20Z
dc.descriptionWe describe a project to study a sample of X-ray luminous clusters of galaxies at redshift z~0.2 at several scales (with HST/WFPC2 and CFHT/CFH12k) and wavebands (optical and X-ray). The main aims of the project are (i) to determine the mass profiles of the clusters on scales ranging from ~10 kpc/h to >1.5 Mpc/h using weak and strong lensing, thereby testing theoretical predictions of a ``universal mass profile'', and (ii) to calibrate the M_tot - T_X relation in view of future application in the study of the evolution of the cluster mass function at higher redshift.
dc.description4 pages, 2 figures, Proceedings of the XXth Moriond Astrophysics Meeting ``Cosmological Physics with Gravitational Lensing'', J.-P. Kneib, Y. Mellier, M. Moniez and J. Tran Thanh Van eds., 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0007131
dc.identifierhttp://arxiv.org/abs/astro-ph/0007131
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1309
dc.subjectAstrophysics
dc.titleA combined HST/CFH12k/XMM survey of X-ray luminous clusters of galaxies at z~0.2
dc.typetext

Files

Collections

arXiv