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20032026
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 16k across the 240 of their papers we have counts for

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Showing 2009 · astro-ph.HEShow all

8 papers · 2 filters

astro-ph.HE2009★ 27 cited

GRB 090313: X-shooter's first shot at a GRB

A. de Ugarte Postigo, P. Goldoni, C. C. Thöne +26

Context. X-shooter is the first second-generation instrument to become operative at the ESO Very Large Telescope (VLT). It is a broad-band medium-resolution spectrograph designed w…

astro-ph.HE2009★ 93 cited

GRB090426: the farthest short gamma-ray burst?

L. A. Antonelli, P. D Avanzo, R. Perna +23

Aims. With an observed and rest-frame duration of < 2s and < 0.5s, respectively, GRB090426 could be classified as a short GRB. The prompt detection, both from space and ground-base…

astro-ph.HE2009★ 39 cited

Testing GRB models with the afterglow of GRB 090102

B. Gendre, A. Klotz, E. Palazzi +9

We present the observations of the afterglow of gamma-ray burst GRB 090102. Optical data taken by the TAROT, REM, GROND, together with publicly available data from Palomar, IAC and…

astro-ph.HE2009★ 4 cited

GRB090111: extra soft steep decay emission and peculiar re-brightening

R. Margutti, T. Sakamoto, G. Chincarini +8

We present a detailed study of GRB090111, focusing on its extra soft power-law photon index Gamma>5 at the very steep decay phase emission (power-law index alpha=5.1, steeper than…

astro-ph.HE2009★ 23 cited

Detailed Radio to Soft Gamma-ray Studies of the 2005 Outburst of the New X-ray Transient XTE J1818-245

M. Cadolle Bel, L. Prat, J. Rodriguez +11

XTE J1818-245 is an X-ray nova that experienced an outburst in 2005, first seen by the RXTE satellite. The source was observed simultaneously at various wavelengths up to soft gamm…

astro-ph.HE2009★ 61 cited

Rise and fall of the X-ray flash 080330: an off-axis jet?

C. Guidorzi, C. Clemens, S. Kobayashi +31

X-ray flashes (XRFs) are a class of gamma-ray bursts (GRBs) with the peak energy of the time-integrated spectrum, Ep, below 30 keV, whereas classical GRBs have Ep of a few hundreds…