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

Oliver Czoske·Jean-Paul Kneib·Ian Smail·Graham P. Smith·Harald Ebeling
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Abstract

We 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.

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Oliver Czoske, Jean-Paul Kneib, Ian Smail, Graham P. Smith, Harald Ebeling. 2000-07-11. A combined HST/CFH12k/XMM survey of X-ray luminous clusters of galaxies at z~0.2. https://arxiv.org/abs/astro-ph/0007131

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