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20052022
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 4.5k across the 43 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 34 cited

The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125

Adria C. Updike, Joshua B. Haislip, Melissa C. Nysewander +52

We report on multi-wavelength observations, ranging from the X-ray to radio wave bands, of the IPN-localized gamma-ray burst GRB 070125. Spectroscopic observations reveal the prese…

astro-ph2008

The hidden X-ray breaks in afterglow light curves

P. A. Curran, A. J. van der Horst, R. A. M. J. Wijers +1

Gamma-Ray Burst (GRB) afterglow observations in the Swift era have a perceived lack of achromatic jet breaks compared to the BeppoSAX, or pre-Swift era. Specifically, relatively fe…

astro-ph2007★ 35 cited

Are the missing X-ray breaks in Gamma-ray Burst afterglow light curves merely hidden?

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

Gamma-ray burst afterglow observations in the Swift era have a perceived lack of achromatic jet breaks compared to the BeppoSAX, or pre-Swift era. Specifically, relatively few brea…

astro-ph2007★ 40 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-ph2007★ 32 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-ph2007★ 81 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…