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20012005
most citedFrom BeppoSAX to INTEGRAL: PDS observations of hard X-ray sources detected in the IBIS survey

3 citations · 6 across the 5 of their papers we have counts for

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8 papers · 1 filter

astro-ph20053 cited

Exploring the Hard X-/soft gamma-ray Continuum Spectra with Laue Lenses

F. Frontera, A. Pisa, P. De Chiara +17

The history of X-ray astronomy has shown that any advancement in our knowledge of the X-ray sky is strictly related to an increase in instrument sensitivity. At energies above 60 k…

astro-ph20043 cited

From BeppoSAX to INTEGRAL: PDS observations of hard X-ray sources detected in the IBIS survey

A. Malizia, L. Bassani, R. Landi +16

The first IBIS galactic plane survey has provided a list of high energy emitting objects above 20 keV; these sources have been detected mostly in the crowded region of the Galactic…

astro-ph2004

The sky behind our galaxy as seen by IBIS on INTEGRAL

L. Bassani, A. Malizia, J. B. Stephen +16

During the Core Programme, INTEGRAL has surveyed a large portion of the sky (around 9000 square degrees); although INTEGRAL is not optimized for extra-galactic studies its observat…

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…

astro-ph2002

IBIS/PICsIT Data and Analysis

J. B. Stephen, L. Foschini, F. Gianotti +12

The imager IBIS on board INTEGRAL is composed of two detector planes: ISGRI (15 keV - 1 MeV) and PICsIT (170 keV - 10 MeV). Here we describe the data structure of PICsIT and the in…

astro-ph2002

First Results from a XMM-Newton Survey of a Distance-Limited (D < 22 Mpc) Sample of Seyfert Galaxies. II - The Galactic Serendipitous Sources

L. Foschini, G. Di Cocco, M. Dadina +9

We present preliminary results from a study with XMM-Newton of the galactic serendipitous sources in a sample of 28 nearby Seyfert galaxies (with D < 22 Mpc). We concentrate here o…