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20002026
most citedA very energetic supernova associated with the gamma-ray burst of 29 March 2003

1.5k citations · 16k across the 206 of their papers we have counts for

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Showing 2006 · astro-phShow all

10 papers · 2 filters

astro-ph2006

Fundamental Properties of GRB-Selected Galaxies: A Swift/VLT Legacy Survey

P. Jakobsson, J. Hjorth, J. P. U. Fynbo +2

We present the motivation, aims and preliminary result from the Swift/VLT legacy survey on gamma-ray burst host galaxies. This survey will produce a homogeneous and well-understood…

astro-ph2006★ 147 cited

HI column densities of z > 2 Swift gamma-ray bursts

P. Jakobsson, J. P. U. Fynbo, C. Ledoux +18

Context: Before the launch of the Swift satellite, the majority of the gamma-ray burst (GRB) afterglows for which Ly-alpha was redshifted into the observable spectrum showed eviden…

astro-ph2006★ 19 cited

Constraints on an optical afterglow and on supernova light following the short burst GRB 050813

P. Ferrero, S. F. Sanchez, D. A. Kann +18

We report early follow-up observations of the error box of the short burst 050813 using the telescopes at Calar Alto and at Observatorio Sierra Nevada (OSN), followed by deep VLT/F…

astro-ph2006★ 447 cited

No supernovae associated with two long-duration gamma ray bursts

Johan P. U. Fynbo, Darach Watson, Christina C. Thoene +28

It is now accepted that long duration gamma-ray bursts (GRBs) are produced during the collapse of a massive star. The standard "collapsar" model predicts that a broad-lined and lum…

astro-ph2006★ 39 cited

Microlensing variability in time-delay quasars

D. Paraficz, J. Hjorth, I. Burud +2

We have searched for microlensing variability in the light curves of five gravitationally lensed quasars with well-determined time delays: SBS 1520+530, FBQ 0951+2635, RX J0911+055…

astro-ph2006★ 164 cited

Supernova 2006aj and the associated X-Ray Flash 060218

J. Sollerman, A. O. Jaunsen, J. P. U. Fynbo +23

We have studied the afterglow of the gamma-ray burst (GRB) of February 18, 2006. This is a nearby long GRB, with a very low peak energy, and is therefore classified as an X-ray Fla…