activity
19972023
most citedDiscovery of the peculiar supernova 1998bw in the error box of GRB980425

1.9k citations · 8.5k across the 172 of their papers we have counts for

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Showing 1997Show all

11 papers · 1 filter

astro-ph1997

Broad band X-ray spectral properties of Gamma-ray bursts with BeppoSAX

F. Frontera, L. Amati, E. Costa +10

In about one year, five gamma-ray bursts were simultaneously observed with the Wide Field Cameras and Gamma Ray Burst Monitor aboard the BeppoSAX satellite. From some of them X-ray…

astro-ph1997★ 2 cited

Hubble Space Telescope Imaging of the Field of GRB970508

E. Pian, A. Fruchter, L. E. Bergeron +15

We report on Hubble Space Telescope observations of the optical transient discovered in the error box of GRB970508. The object was imaged on 1997 June 2 with the Space Telescope Im…

astro-ph1997

BeppoSAX observations of the X-ray binary pulsar 4U1626-67

M. Orlandini, D. Dal Fiume, F. Frontera +6

We report on observations of the low-mass X-ray binary 4U1626-67 performed during the BeppoSAX Science Verification Phase. We present the broad-band 0.1-100 keV pulse averaged spec…

astro-ph1997★ 1 cited

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…

astro-ph1997★ 60 cited

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…

astro-ph1997★ 5 cited

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…