401 citations · 888 across the 10 of their papers we have counts for
10 papers
The Coma Cluster hard X-ray spectrum revisited: still no evidence for a hard tail
M. Rossetti, S. Molendi
In this note, we reply to Fusco-Femiano et al. (2004) and Fusco-Femiano et al. (2006), who cast doubts on our analysis of the PDS observations of the Coma Cluster which we describe…
The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton
Andrea De Luca, Silvano Molendi
We have measured the spectrum of the Cosmic X-ray Background (CXB) in the 2-8 keV range with the high throughput EPIC/MOS instrument onboard XMM-Newton. A large sample of high gala…
High Energy Results from BeppoSAX
R. Fusco-Femiano, D. Dal Fiume, M. Orlandini +5
We review all the BeppoSAX results relative to the search for additional nonthermal components in the spectra of clusters of galaxies. In particular, our MECS data analysis of A219…
X-ray bright optically quiet galaxies: the case of P3
A. Comastri, M. Brusa, P. Ciliegi +10
Recent X-ray surveys have clearly demonstrated that a population of optically dull, X-ray bright galaxies is emerging at X-ray fluxes of the order of 10-14 erg cm-2 s-1. The nature…
The HELLAS2XMM survey: I. The X-ray data and the Log(N)-Log(S)
A. Baldi, S. Molendi, A. Comastri +3
We present the first results from an XMM-Newton serendipitous medium-deep survey, which covers nearly three square degrees. We detect a total of 1022, 495 and 100 sources, down to…
Metallicity Gradients in X-ray Clusters of Galaxies
Sabrina De Grandi, Silvano Molendi
We present the projected metallicity profiles for a sample of 17 rich galaxy clusters observed by BeppoSAX. We find that the 8 non-cooling flow clusters have flat metallicity profi…