activity
19992004
most citedFrom BeppoSAX to INTEGRAL: PDS observations of hard X-ray sources detected in the IBIS survey

3 citations · 4 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph2004

SPI Measurements of the Diffuse Galactic Hard X-ray Continuum

A. W. Strong, R. Diehl, H. Halloin +6

INTEGRAL Spectrometer SPI data from the first year of the Galactic Centre Deep Exposure has been analysed for the diffuse continuum from the Galactic ridge. A new catalogue of sour…

astro-ph20041 cited

Contribution of point sources to the soft gamma-ray Galactic emission

Regis Terrier, Francois Lebrun, Guillaume Belanger +6

The nature of the soft gamma-ray (20-200 keV) Galactic emission has been a matter of debate for a long time. Previous experiments have tried to separate the point source contributi…

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-ph2001

Integral/IBIS Observations of persistent black hole spectral states during the Core Program

P. Laurent, P. Goldoni, A. Goldwurm +1

The Imager on Board the Integral Satellite (IBIS) is one of the two main telescopes of Integral, the ESA soft gamma-ray mission to be launched in 2002. The Integral Core Program wi…

astro-ph2001

Observation of a Black-Hole X-ray Nova in Outburst with INTEGRAL

P. Goldoni, A. Goldwurm, P. Laurent +2

We simulate the observation of a bright Nova Musca-like X-ray nova during outburst with INTEGRAL, the next ESA gamma-ray space observatory. We will show how performances of the INT…

astro-ph1999

Hard X-Rays from the Galactic Nucleus: Present and Future Observations

A. Goldwurm, P. Goldoni, P. Laurent +2

In spite of increasing evidences of the presence of a massive Black Hole at the Galactic Center, its radio counterpart, Sgr A*, shows little activity at high energies, and recent m…