activity
19942009
most citedX-ray spectral properties of AGN in the Chandra Deep Field South

388 citations · 4.3k across the 43 of their papers we have counts for

collaborators
Showing 2003Show all

7 papers · 1 filter

astro-ph2003

Scaling laws in X-ray Galaxy Clusters at redshift between 0.4 and 1.3

S. Ettori, P. Tozzi, S. Borgani +1

(Abriged) We present a study of the integrated physical properties of a sample of 28 X-ray galaxy clusters observed with Chandra at redshift between 0.4 and 1.3. In particular, we…

astro-ph2003

X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation

S. Borgani, G. Murante, V. Springel +6

We present results on the X-ray properties of clusters and groups of galaxies, extracted from a large hydrodynamical simulation. We used the GADGET code to simulate a LambdaCDM mod…

astro-ph2003

Chandra and XMM-Newton Observations of RDCS1252.9-2927, A Massive Cluster at z=1.24

P. Rosati, P. Tozzi, S. Ettori +10

We present deep Chandra and XMM obervations of the galaxy cluster RDCS1252.9-2927, which was selected from the ROSAT Deep Cluster Survey (RDCS) and confirmed by extensive spectrosc…

astro-ph2003

Iron abundance in the ICM at high redshift

P. Tozzi, P. Rosati, S. Ettori +3

We present the analysis of the X-ray spectra of 18 distant clusters of galaxies with redshift 0.3 < z < 1.3. Most of them were observed with the Chandra satellite in long exposures…

astro-ph2003

Tracing the large scale structure in the Chandra Deep Field South

R. Gilli, A. Cimatti, E. Daddi +16

We report the discovery of large scale structures of X-ray sources in the 1Msec observation of the Chandra Deep Field South. Two main structures appear as narrow (Delta_z < 0.02) s…

astro-ph2003

Cooling and heating the ICM in hydrodynamical simulations

L. Tornatore, S. Borgani, V. Springel +3

We discuss Tree+SPH simulations of galaxy clusters and groups, aimed at studying the effect of cooling and non-gravitational heating on observable properties of the ICM. We simulat…