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19992005
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astro-ph2005

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…

astro-ph2003

An XMM and Chandra view of massive clusters of galaxies to z=1

L. R. Jones, B. J. Maughan, H. Ebeling +7

The X-ray properties of a sample of high redshift (z>0.6), massive clusters observed with XMM-Newton and Chandra are described, including two exceptional systems. One, at z=0.89, h…

astro-ph2002

In-orbit calibration of vignetting in XMM-Newton EPIC

D. H. Lumb

We briefly describe the in orbit measurements of the mirror vignetting, using observations of SNR G21.5-09. The instrument features which complicate these measurements are briefly…

astro-ph2002

XMM-Newton EPIC in orbit background

D. H. Lumb

We briefly describe the methods used in compiling a set of high galactic latitude background data. The characteristics and limitations of the data which affect their use as a templ…

astro-ph2002

XMM-Newton calibration - an overview

D. H. Lumb

This paper introduces the articles that describe detailed aspects of the XMM-Newton calibration. The unique calibration issues of XMM-Newton are highlighted. The original calibrati…

astro-ph2002

Timing study of the isolated neutron star RX J0720.4-3125

Silvia Zane, Frank Haberl, Mark Cropper +4

We present a combined analysis of XMM-Newton, Chandra and Rosat observations of the isolated neutron star RX J0720.4-3125, spanning a total period of \sim 7 years. We develop a max…