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20082021
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408 citations · 2.6k across the 25 of their papers we have counts for

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Showing 2011Show all

6 papers · 1 filter

astro-ph.HE2011★ 69 cited

The Fast Evolution of SN 2010bh associated with XRF 100316D

Felipe Olivares E., Jochen Greiner, Patricia Schady +13

(...) Since 1998, only half a dozen spectroscopically confirmed associations have been discovered and XRF 100316D associated with the type-Ic SN 2010bh at z = 0.059 is among the la…

astro-ph.CO2011★ 110 cited

Super-solar Metal Abundances in Two Galaxies at z ~ 3.57 revealed by the GRB 090323 Afterglow Spectrum

S. Savaglio, A. Rau, J. Greiner +12

We report on the surprisingly high metallicity measured in two absorption systems at high redshift, detected in the Very Large Telescope spectrum of the afterglow of the gamma-ray…

astro-ph.HE2011★ 73 cited

GRB 091127: The cooling break race on magnetic fuel

Robert Filgas, Jochen Greiner, Patricia Schady +13

Using high-quality, broad-band afterglow data for GRB 091127, we investigate the validity of the synchrotron fireball model for gamma-ray bursts, and infer physical parameters of t…

astro-ph.CO2011★ 184 cited

The SEDs and Host Galaxies of the dustiest GRB afterglows

T. Krühler, J. Greiner, P. Schady +18

(Abridged) Until recently the information inferred from gamma-ray burst follow-up observations was mostly limited to optically bright afterglows, biasing all demographic studies ag…

astro-ph.HE2011★ 61 cited

On the nature of the extremely fast optical rebrightening of the afterglow of GRB 081029

M. Nardini, J. Greiner, T. Kruehler +14

Context. After the launch of the Swift satellite, the Gamma-Ray Burst (GRB) optical light-curve smoothness paradigm has been questioned thanks to the faster and better sampled opti…

astro-ph.HE2011★ 8 cited

GRB 071028B, a burst behind large amounts of dust in an unabsorbed galaxy

C. Clemens, J. Greiner, T. Krühler +12

We report on the discovery and properties of the fading afterglow and underlying host galaxy of GRB 071028B, thereby facilitating a detailed comparison between these two. Observati…