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10 papers
project: III. Gas mass fraction shape in high redshift clusters
Rachida Sadat, Alain Blanchard, Sebastien C. Vauclair +10
We study the gas mass fraction, behavior in project. The typical shape of high redshift galaxy clusters follows the global shape inf…
The XMM--NEWTON Omega Project: II.Cosmological implications from the high redshift L-T relation of X-ray clusters
S. C. Vauclair, A. Blanchard, R. Sadat +7
The evolution with redshift of the temperature-luminosity relation of X-ray galaxy clusters is a key ingredient to break degeneracies in the interpretation of X-ray clusters redshi…
The XMM--NEWTON Omega Project: I. The X-ray Luminosity - Temperature Relation at z>0.4
D. H. Lumb, J. G. Bartlett, A. K. Romer +9
(abridged) We describe XMM-Newton Guaranteed Time observations of a sample of eight high redshift (0.45<z<0.62) clusters. The goal of these observations was to measure the luminosi…
Measuring the matter distribution within z=0.2 cluster lenses with XMM-Newton
P. B. Marty, J. -P. Kneib, R. Sadat +4
We present an analysis of 7 clusters observed by XMM as part of our survey of 17 most X-ray luminous clusters of galaxies at z=0.2 selected for a comprehensive and unbiased study o…
Data analysis methods for XMM-Newton observations of extended sources. Application to bright massive clusters of galaxies at z=0.2
Philippe B. Marty, Jean-Paul Kneib, Rachida Sadat +2
In this paper, a review is given of methods useful for XMM-Newton EPIC data analysis of extended sources, along with some applications to a bright massive cluster of galaxies at z=…
The Diabolo photometer and the future of ground-based millimetric bolometer devices
F. -X. Desert, A. Benoit, Ph. Camus +9
The millimetric atmospheric windows at 1 and 2 mm are interesting targets for cosmological studies. Two broad areas appear leading this field: 1) the search for high redshift star-…