activity
19972004
most citedStudy of Unidentified EGRET sources with INTEGRAL: first results and future prospects

1 citations · 1 across the 8 of their papers we have counts for

collaborators

18 papers

astro-ph2004

Chandra observations of X-ray source overdensities in distant galaxy cluster fields

N. Cappelluti, M. Cappi, M. Dadina +4

The first systematic study of the serendipitous X-ray source density around 10 high z (0.24<z<1.2) clusters performed with Chandra is presented. A factor \~2 overdensity has been f…

astro-ph2004

INTEGRAL monitoring of the Black Hole candidate 1E 1740.7-2942

M. Del Santo, A. Bazzano, D. M. Smith +24

The brightest persistent Galactic black hole candidate close to the Galactic Centre, 1E 1740.7-2942, has long been observed with INTEGRAL. In this paper, we report on the long-term…

astro-ph20041 cited

Study of Unidentified EGRET sources with INTEGRAL: first results and future prospects

G. Di Cocco, A. J. Castro-Tirado, S. Chaty +12

The primary objective of the study of unidentified EGRET sources with INTEGRAL is to locate with a few arcminute accuracy the hard X-ray / soft gamma-ray counterparts within the EG…

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-ph2003

Search for relativistic beaming in ultraluminous X-ray sources

L. Foschini, G. Malaguti, G. Di Cocco +3

The nature of the ultraluminous X-ray sources (ULX) is still to be understood. Several hypotheses have been suggested to explain the high X-ray luminosity: stellar mass black holes…

astro-ph2002

Search for ultraluminous X-ray sources in nearby galaxies

L. Foschini, G. Di Cocco, L. C. Ho +9

Little is presently known about the nature of ultraluminous X-ray sources (ULX). Different hypotheses have been proposed to explain their properties: intermediate-mass BHs, Kerr BH…