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Chapter and Conference Paper
Exploring Massive Galaxy Clusters: XMM-Newton observations of two morphology unbiased samples at z ∼ 0.2 and z ∼ 0.3
For the spectral determination of the temperature distribution in galaxy clusters we developed a double background subtraction method, and applied it to 2 morphology unbiased samples of X-ray luminous galaxy c...
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Chapter and Conference Paper
Statistics of X-ray Observables of Cooling Core and Non-cooling Core Clusters of Galaxies
In this poster we study the segregation of Cooling Core (CC) and Non-Cooling Core (NCC) clusters in the LX–T, LX–M and M–T relation using the HIFLUGCS sample ([1]). A major goal in this study is to better unde...