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20032005
most citedEvolution of the polarization of the optical afterglow of the gamma-ray burst GRB 030329

116 citations

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6 papers · 1 filter

astro-ph200766 cited

Detection of GRB 060927 at z = 5.47: Implications for the Use of Gamma-Ray Bursts as Probes of the End of the Dark Ages

A. E. Ruiz-Velasco, H. Swan, E. Troja +54

We report on follow-up observations of the GRB 060927 using the ROTSE-IIIa telescope and a suite of larger aperture ground-based telescopes. An optical afterglow was detected 20 s…

astro-ph2005

Weibel Instability Driven by Relativistic Pair Jets: Particle Acceleration, Magnetic Field Generation, and Emission

K. -I. Nishikawa, P. Hardee, C. B. Hededal +4

Shock acceleration is a ubiquitous phenomenon in astrophysical plasmas. Plasma waves and their associated instabilities (e.g., Buneman, Weibel and other two-stream instabilities) c…

astro-ph200413 cited

Massive star-formation rates of gamma-ray burst host galaxies: an unobscured view in X-rays

D. Watson, J. Hjorth, P. Jakobsson +3

The hard X-ray (2-10keV) luminosity of a star-forming galaxy tracks its population of high mass X-ray binaries and is essentially unobscured. It is therefore a practically unbiased…

astro-ph200425 cited

Soft Gamma Repeaters and Anomalous X-ray Pulsars: Magnetar Candidates

P. M. Woods, C. Thompson

This article is a review of Soft Gamma Repeaters and Anomalous X-ray Pulsars. It contains a brief historical record of the emergence of these classes of neutron stars, a thorough o…

astro-ph200435 cited

Small-scale variations in the radiating surface of the GRB 011211 jet

P. Jakobsson, J. Hjorth, E. Ramirez-Ruiz +12

We report the discovery of the afterglow of the X-ray rich, long-duration gamma-ray burst GRB 011211 and present evidence for oscillatory behaviour in its early optical light curve…

astro-ph2003116 cited

Evolution of the polarization of the optical afterglow of the gamma-ray burst GRB 030329

J. Greiner, S. Klose, K. Reinsch +23

We report 31 polarimetric observations of the afterglow of GRB 030329 with high signal-to-noise and high sampling frequency. We establish the polarization light curve, detect susta…