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19972003
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astro-ph2003

The Ultra Luminous Infrared Galaxy MKN 231: New clues from BeppoSAX and XMM-Newton

V. Braito, R. Della Ceca, E. Piconcelli +11

We present BeppoSAX and XMM-Newton observations of MKN 231. These observations and in particular the BeppoSAX PDS data allowed us to unveil, for the first time, the highly absorbed…

astro-ph2002

An XMM-Newton Survey of Ultra-Luminous Infrared Galaxies

V. Braito, A. Franceschini, R. Della Ceca +8

We present preliminary results of XMM-Newton observations of 5 Ultra-luminous Infrared Galaxies (ULIRGs), part of a mini-survey program dedicated to 10 ULIRGs selected from the bri…

astro-ph2001

Relic Black Holes and Type 2 Quasars

Alessandro Marconi, Marco Salvati

We follow the evolution of the Black Hole mass function in the assumption that mass accretion onto a massive BH is the powering mechanism of AGN activity. With reasonable assumptio…

astro-ph2001

HST Imaging in the Chandra Deep Field South: I. Multiple AGN Populations

E. J. Schreier, A. M. Koekemoer, N. A. Grogin +9

We present preliminary results from imaging three HST/WFPC2 fields in V and I within the Chandra Deep Field South (CDFS). HST's sensitivity and resolution are sufficient to reveal…

astro-ph2000

Sub-mm and X-ray background: two unrelated phenomena?

P. Severgnini, R. Maiolino, M. Salvati +9

Obscured AGNs are thought to contribute a large fraction of the hard X-ray background (2-10 keV), and have also been proposed as the powerhouse of a fraction of the SCUBA sources w…

astro-ph2000

The hard X-ray emission of luminous infrared galaxies

G. Risaliti, R. Gilli, R. Maiolino +1

We present a study of the hard X-ray properties of a sample that includes all the Luminous Infrared Galaxies (LIGs, L_IR > 10^11 L_sun) observed in the 2-10 keV energy band (new an…