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What can BeppoSAX do about the 2-10 keV cosmic background ? A progress report
L. Chiappetti, G. Cusumano, S. Del Sordo +3
We report the current status of the analysis of the MECS background using the entire dataset of the BeppoSAX Science performance Verification Phase. We have collected 360 ks of dar…
The pulsed light curves of Her X-1 as observed by BeppoSAX
D. Dal Fiume, M. Orlandini, G. Cusumano +8
We report on the timing analysis of the observation of the X-ray binary pulsar Her X-1 performed during the BeppoSAX Science Verification Phase. The observation covered more that t…
Spectral Properties of the Prompt X-ray emission and Afterglow from the Gamma-Ray Burst of 28 February 1997
F. Frontera, E. Costa, L. Piro +18
We report high-energy spectral data of the prompt emission of GRB970228 and its X-ray afterglow. We establish that the nature of the X-ray afterglow emission is non-thermal and sim…
The Vela X-1 pulse-averaged spectrum as observed by BeppoSAX
M. Orlandini, D. Dal Fiume, F. Frontera +7
We report on the 20 ksec observation of Vela X-1 performed by BeppoSAX on 1996 July 14 during its Science Verification Phase. We observed the source in two intensity states, charac…
Final performances of the X-ray Mirrors of the JET-X telescope
E. Poretti, S. Campana, O. Citterio +10
The Joint European Telesscope (JET-X) is one of the core scientific instruments of the SPECTRUM-X-Gamma mission. JET-X was designed to study X-ray emissions in the band 0.3-10 KeV.…
BeppoSAX observation of the X-ray binary pulsar Vela X-1
M. Orlandini, D. Dal Fiume, L. Nicastro +7
We report on the spectral (pulse averaged) and timing analysis of the ~ 20 ksec observation of the X-ray binary pulsar Vela X-1 performed during the BeppoSAX Science Verification P…