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20042026
most citedThe Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars

765 citations · 11.8k across the 178 of their papers we have counts for

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Showing 2008Show all

15 papers · 1 filter

astro-ph2008★ 220 cited

GRB 080913 at redshift 6.7

J. Greiner, T. Kruehler, J. P. U. Fynbo +44

We report on the detection by Swift of GRB 080913, and subsequent optical/near-infrared follow-up observations by GROND which led to the discovery of its optical/NIR afterglow and…

astro-ph2008★ 29 cited

Simultaneous polarization monitoring of supernovae SN2008D/XT080109 and SN2007uy: isolating geometry from dust

J. Gorosabel, A. de Ugarte Postigo, A. J. Castro-Tirado +16

The possible existence of a continuum encompassing the diversity of explosive stellar deaths,ranging from ordinary SNe to relativistic hypernovae associated with long duration GRBs…

astro-ph2008★ 42 cited

Optical and infrared flares from a transient Galactic soft gamma-ray repeater

A. J. Castro-Tirado, A. de Ugarte Postigo, J. Gorosabel +33

Soft gamma-ray repeaters (SGRs) are a rare type of gamma-ray transient sources that are ocasionally detected as bursts in the high-energy sky. They are thought to be produced by ma…

astro-ph2008★ 47 cited

On Dust Extinction of Gamma-ray Burst Host Galaxies

Aigen Li, S. L. Liang, D. A. Kann +3

Although it is well recognized that gamma-ray burst (GRB) afterglows are obscured and reddened by dust in their host galaxies, the wavelength-dependence and quantity of dust extinc…

astro-ph2008

Can optical afterglows be used to discriminate between Type I and Type II GRBs?

D. A. Kann

The precise localization of short/hard (Type I) gamma-ray bursts (GRBs) in recent years has answered many questions but raised even more. I present some results of a systematic stu…

astro-ph2008★ 52 cited

Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z=3.2 gamma-ray burst

C. C. Thöne, D. A. Kann, G. Jóhannesson +58

Aims: With this paper we want to investigate the highly variable afterglow light curve and environment of gamma-ray burst (GRB) 060526 at . Methods: We present one of the…