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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 2014Show all

15 papers · 1 filter

astro-ph.HE2014★ 91 cited

Comparing the spectral lag of short and long gamma-ray bursts and its relation with the luminosity

M. G. Bernardini, G. Ghirlanda, S. Campana +14

We investigated the rest frame spectral lags of two complete samples of bright long (50) and short (6) gamma-ray bursts (GRB) detected by Swift. We analysed the Swift/BAT data thro…

astro-ph.HE2014★ 105 cited

Circular polarization in the optical afterglow of GRB 121024A

K. Wiersema, S. Covino, K. Toma +37

Gamma-ray bursts (GRBs) are most probably powered by collimated relativistic outflows (jets) from accreting black holes at cosmological distances. Bright afterglows are produced wh…

astro-ph.GA2014★ 55 cited

The mysterious optical afterglow spectrum of GRB140506A at z=0.889

J. P. U. Fynbo, T. Krühler, K. Leighly +40

Context. Gamma-ray burst (GRBs) afterglows probe sightlines to star-forming regions in distant star-forming galaxies. Here we present a study of the peculiar afterglow spectrum of…

astro-ph.HE2014★ 139 cited

Are LGRBs biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of LGRBs. I: Stellar mass at z<1

S. D. Vergani, R. Salvaterra, J. Japelj +20

LGRBs are associated with massive stars and are therefore linked to star formation. The conditions necessary to produce LGRBs can affect the relation between the LGRB rate and star…

astro-ph.GA2014★ 83 cited

The warm, the excited, and the molecular gas: GRB 121024A shining through its star-forming galaxy

M. Friis, A. De Cia, T. Krühler +28

We present the first reported case of the simultaneous metallicity determination of a gamma-ray burst (GRB) host galaxy, from both afterglow absorption lines as well as strong emis…

astro-ph.GA2014★ 40 cited

VLT/X-shooter spectroscopy of the afterglow of the Swift GRB 130606A: Chemical abundances and reionisation at

O. E. Hartoog, D. Malesani, J. P. U. Fynbo +28

The reionisation of the Universe is thought to have ended around z~6, as inferred from spectroscopy of distant bright background sources, such as quasars (QSO) and gamma-ray burst…