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20082018
most citedGROND - a 7-channel imager

408 citations · 862 across the 10 of their papers we have counts for

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7 papers · 1 filter

astro-ph.HE2018★ 30 cited

The luminous host galaxy, faint supernova and rapid afterglow rebrightening of GRB 100418A

A. de Ugarte Postigo, C. C. Thoene, K. Bensch +35

Long gamma-ray bursts give us the chance to study both their extreme physics and the star-forming galaxies in which they form. GRB 100418A, at a z = 0.6239, had a bright optical an…

astro-ph.HE2017★ 31 cited

Late-time observations of the relativistic tidal disruption flare candidate Swift J1112.2-8238

G. C. Brown, A. J. Levan, E. R. Stanway +6

We present late-time follow-up of the relativistic tidal disruption flare candidate Swift J1112.2-8238. We confirm the previously determined redshift of based o…

astro-ph.HE2017★ 58 cited

Investigating the diversity of supernovae type Iax: A MUSE and NOT spectroscopic study of their environments

J. D. Lyman, F. Taddia, M. D. Stritzinger +9

SN 2002cx-like Type Ia supernovae (also known as SNe Iax) represent one of the most numerous peculiar SN classes. They differ from normal SNe Ia by having fainter peak magnitudes,…

astro-ph.HE2017★ 37 cited

A long optical plateau in the afterglow of the Extended Emission short GRB 150424A: Evidence for energy injection by a magnetar?

F. Knust, J. Greiner, H. J. van Eerten +14

Short-duration GRBs with extended emission form a subclass of short GRBs, comprising about 15% of the short-duration sample. Afterglow detections of short GRBs are also rare (about…

astro-ph.HE2010★ 18 cited

GRB 050502B optical afterglow: a jet break at high redshift

P. Afonso, J. Greiner, E. Pian +9

Aims: GRB 050502B is well known for the very bright flare displayed in its X-ray light curve. Despite extensive studies, however, the optical light curve has never been discussed a…

astro-ph.HE2009★ 61 cited

Rise and fall of the X-ray flash 080330: an off-axis jet?

C. Guidorzi, C. Clemens, S. Kobayashi +31

X-ray flashes (XRFs) are a class of gamma-ray bursts (GRBs) with the peak energy of the time-integrated spectrum, Ep, below 30 keV, whereas classical GRBs have Ep of a few hundreds…