SWIFT / XRT FOLLOW-UP OBSERVATIONS OF INTEGRAL AGNS R. Landi, A. Malizia, L. Bassani , N. Masetti, J.B. Stephen, F.Gianotti, F. Schiavone 1 , A. Bazzano, P. Ubertini 2 , A. J. Bird, A. J. Dean3 , and R. Walter4 IASF-INAF, Bologna, Italy 2 IASF- INAF, Roma, Italy 3 University of Southampton, Southampton, UK INTEGRAL Science Data Centre, Versoix, Switzerland 1 4 ABSTRACT In five years of operation, data from ... In this work we present X-ray data (0.2­10 keV) for a set of 8 identified with AGN. ...

Lack of co oling flow clusters at z 0.5 A. Vikhlinin1,2 , R. Burenin2 , W. R. Forman1 , C. Jones1 , A. Hornstrup3 , S. S. Murray1, and H. Quintana4 1 2 3 4 Harvard-Smithsonian ... Astronomia y Astrofisica, Pontificia Universidad Catolica de Chile The goal of this work is to study the incidence rate of co oling flows in the high redshift clusters using Chandra observations of z 0.5 ob jects from a new large, ... Fig. ... Lack of "cooling flow" clusters at z > 0.5 3 Fig. ...