activity
19992009
most citedAn optical supernova associated with the X-ray flash XRF 060218

544 citations · 1.5k across the 20 of their papers we have counts for

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Showing 2007Show all

8 papers · 1 filter

astro-ph200740 cited

The host of GRB 060206: kinematics of a distant galaxy

Christina C. Thoene, Klaas Wiersema, Cedric Ledoux +13

We present early (starting 1.6h after the burst) WHT/ISIS optical spectroscopy of the afterglow of the gamma-ray burst GRB 060206 detecting a range of metal absorption lines and th…

astro-ph200732 cited

GRB 060206 and the quandary of achromatic breaks in afterglow light curves

P. A. Curran, A. J. van der Horst, R. A. M. J. Wijers +20

Gamma-ray burst afterglow observations in the Swift era have a perceived lack of achromatic jet breaks compared to the BeppoSAX era. We present our multi-wavelength analysis of GRB…

astro-ph200726 cited

Spectroscopy and multiband photometry of the afterglow of intermediate duration gamma-ray burst 040924 and its host galaxy

K. Wiersema, A. J. van der Horst, D. A. Kann +19

We present optical photometry and spectroscopy of the afterglow and host galaxy of gamma-ray burst 040924. This GRB had a rather short duration of T90 ~2.4s, and a well sampled opt…

astro-ph20077 cited

GRB 030329: 3 years of radio afterglow monitoring

A. J. van der Horst, A. Kamble, R. A. M. J. Wijers +7

Radio observations of gamma-ray burst (GRB) afterglows are essential for our understanding of the physics of relativistic blast waves, as they enable us to follow the evolution of…

astro-ph200781 cited

Detailed study of the GRB 030329 radio afterglow deep into the non-relativistic phase

A. J. van der Horst, A. Kamble, L. Resmi +8

We explore the physics behind one of the brightest radio afterglows ever, GRB 030329, at late times when the jet is non-relativistic. We determine the physical parameters of the bl…

astro-ph200761 cited

A case of mistaken identity? GRB 060912A and the nature of the long -- short GRB divide

A. J. Levan, P. Jakobsson, C. Hurkett +13

We investigate the origin of the GRB 060912A, which has observational properties that make its classification as either a long or short burst ambiguous. Short duration GRBs (SGRBs)…