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20032026
most citedCompact radio emission indicates a structured jet was produced by a binary neutron star merger

395 citations · 7.9k across the 156 of their papers we have counts for

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Showing 2011Show all

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astro-ph.HE2011★ 89 cited

The X-ray absorbing column density of a complete sample of bright Swift Gamma-Ray Bursts

S. Campana, R. Salvaterra, A. Melandri +7

A complete sample of bright Swift Gamma-ray Bursts (GRBs) has been recently selected by Salvaterra et al. (2011). The sample has a high level of completeness in redshift (91%). We…

astro-ph.HE2011★ 60 cited

The Dark Bursts population in a complete sample of bright Swift Long Gamma-Ray Bursts

A. Melandri, B. Sbarufatti, P. D'Avanzo +11

We study the properties of the population of optically dark events present in a carefully selected complete sample of bright Swift long gamma-ray bursts. The high level of complete…

astro-ph.HE2011★ 176 cited

A complete sample of bright Swift Long Gamma Ray Bursts: testing the spectral-energy correlations

L. Nava, R. Salvaterra, G. Ghirlanda +11

We use a nearly complete sample of Gamma Ray Bursts (GRBs) detected by the Swift satellite to study the correlations between the spectral peak energy Ep of the prompt emission, the…

astro-ph.CO2011★ 249 cited

A complete sample of bright Swift Long Gamma-Ray Bursts: Sample presentation, Luminosity Function and evolution

R. Salvaterra, S. Campana, S. D. Vergani +11

We present a carefully selected sub-sample of Swift Long Gamma-ray Bursts (GRBs), that is complete in redshift. The sample is constructed by considering only bursts with favorable…

astro-ph.HE2011★ 135 cited

The Highly Energetic Expansion of SN2010bh Associated with GRB 100316D

Filomena Bufano, Elena Pian, Jesper Sollerman +50

We present the spectroscopic and photometric evolution of the nearby (z = 0.059) spectroscopically confirmed type Ic supernova, SN 2010bh, associated with the soft, long-duration g…