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Non-thermal emission in the core of Perseus: results from a long XMM-Newton observation
Silvano Molendi, Fabio Gastaldello
We employ a long XMM-Newton observation of the core of the Perseus cluster to validate claims of a non-thermal component discovered with Chandra. From a meticulous analysis of our…
Radial metallicity profiles for a large sample of galaxy clusters observed with XMM-Newton
A. Leccardi, S. Molendi
Aims. We measured radial metallicity profiles for a sample of ~50 hot, intermediate redshift galaxy clusters, selected from the XMM-Newton archive. Methods. As in our previous pape…
Radial temperature profiles for a large sample of galaxy clusters observed with XMM-Newton
A. Leccardi, S. Molendi
Aims. We measure, as far out as possible, radial temperature profiles for a sample of ~50 hot, intermediate redshift galaxy clusters, selected from the XMM-Newton archive, keeping…
The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
G. Hasinger, N. Cappelluti, H. Brunner +21
We present the first set of XMM-Newton EPIC observations in the 2 square degree COSMOS field. The strength of the COSMOS project is the unprecedented combination of a large solid a…
A cluster in a crowded environment: XMM-Newton and Chandra observations of A3558
M. Rossetti, S. Ghizzardi, S. Molendi +1
Combining XMM-Newton and Chandra data, we have performed a detailed study of Abell 3558. Our analysis shows that its dynamical history is more complicated than previously thought.…
Searching for Sharp Surface Brightness Discontinuities: a Systematic Study of Cold Fronts in Galaxy Clusters
S. Ghizzardi, S. Molendi, A. Leccardi +1
We perform a systematic search of cold fronts in a sample of 62 clusters observed with XMM-Newton with redshift ranging from 0.01 to 0.3. We detect one or more cold fronts in 21 (3…