activity
20052026
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 10.7k across the 140 of their papers we have counts for

collaborators
Showing 2011Show all

10 papers · 1 filter

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★ 67 cited

A minor body falling onto a neutron star as an explanation for the unusual gamma-ray burst GRB 101225A

S. Campana, G. Lodato, P. D'Avanzo +17

The tidal disruption of a solar mass star around a supermassive black hole has been extensively studied analytically and numerically. In these events the star develops into an elon…

astro-ph.HE2011★ 170 cited

Gamma Ray Bursts in the comoving frame

G. Ghirlanda, L. Nava, G. Ghisellini +4

We estimate the bulk Lorentz factor Gamma_0 of 31 GRBs using the measured peak time of their afterglow light curves. We consider two possible scenarios for the estimate of Gamma_0:…