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19972008
most citedExploring the Hard X-/soft gamma-ray Continuum Spectra with Laue Lenses

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

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astro-ph20081 cited

Comments to the review "Nonthermal phenomena in clusters of galaxies" by Y.Rephaeli et al. that will appear on the book: Clusters of galaxies: beyond the thermal view

Roberto Fusco-Femiano, Mauro Orlandini

Comments to the review "Nonthermal Phenomena in Clusters of Galaxies" by Y.Rephaeli et al. (arXiv:0801.0982 [astro-ph]) that regard the presence of a hard X-ray excess in the Coma…

astro-ph2005

The BeppoSAX view on the galactic high-mass X-ray binary 4U 0114+65

N. Masetti, M. Orlandini, D. Dal Fiume +5

A pointed observation on the galactic high-mass X-ray binary 4U 0114+65 was carried out with BeppoSAX in order to compare the X-ray spectral and timing characteristics observed by…

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-ph2004

Hard X-ray emission from Serpens X-1 as observed by INTEGRAL

N. Masetti, L. Foschini, E. Palazzi +5

We here report results of an INTEGRAL observation of the X-ray burst and atoll source Ser X-1 performed on May 2003. The object was observed for a total of 400 ks but nearly 8 degr…

astro-ph2002

Strongly absorbed quiescent X-ray emission from the X-ray transient XTE J0421+56

L. Boirin, A. N. Parmar, D. Lumb +2

We have observed the soft X-ray transient XTE J0421+56 in quiescence with XMM-Newton. The observed spectrum is highly unusual being dominated by a broad feature at 6.5 keV and can…

astro-ph2000

Hard X-rays from Type II bursts of the Rapid Burster and its transition toward quiescence

N. Masetti, F. Frontera, L. Stella +10

We report on 4 BeppoSAX Target Of Opportunity observations of MXB 1730-335, the Rapid Burster (RB), made during the 1998 February-March outburst. In the first observation, approxim…