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20112024
most citedA very luminous magnetar-powered supernova associated with an ultra-long gamma-ray burst

303 citations · 2k across the 37 of their papers we have counts for

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astro-ph.HE2024

The GROND gamma-ray burst sample. I. Overview and statistics

J. Greiner, T. Krühler, J. Bolmer +17

A dedicated gamma-ray burst (GRB) afterglow observing program was performed between 2007 and 2016 with GROND, a seven-channel optical and near-infrared imager at the 2.2m telescope…

astro-ph.HE2017★ 45 cited

The Optical/NIR afterglow of GRB 111209A: Complex yet not Unprecedented

D. A. Kann, P. Schady, F. Olivares E. +24

Afterglows of Gamma-Ray Bursts (GRBs) are simple in the most basic model, but can show many complex features. The ultra-long duration GRB 111209A, one of the longest GRBs ever dete…

astro-ph.HE2016★ 53 cited

Highly Luminous Supernovae associated with Gamma-Ray Bursts I.: GRB 111209A/SN 2011kl in the Context of Stripped-Envelope and Superluminous Supernovae

D. A. Kann, P. Schady, F. E. Olivares +22

GRB 111209A, one of the longest Gamma-Ray Bursts (GRBs) ever observed, is linked to SN 2011kl, the most luminous GRB-Supernova (SN) detected so far, which shows evidence for being…

astro-ph.HE2015★ 303 cited

A very luminous magnetar-powered supernova associated with an ultra-long gamma-ray burst

Jochen Greiner, Paolo A. Mazzali, D. Alexander Kann +29

A new class of ultra-long duration (>10,000 s) gamma-ray bursts has recently been suggested. They may originate in the explosion of stars with much larger radii than normal long ga…

astro-ph.HE2015★ 15 cited

Microphysics and dynamics of the Gamma-Ray Burst 121024A

K. Varela, H. van Eerten, J. Greiner +28

Aims. The aim of the study is to constrain the physics of gamma-ray bursts (GRBs) by analysing the multi-wavelength afterglow data set of GRB 121024A that covers the full range fro…

astro-ph.HE2015★ 63 cited

Gamma-Ray Bursts Trace UV Metrics of Star Formation over 3 < z < 5

Jochen Greiner, Derek B. Fox, Patricia Schady +15

We present the first uniform treatment of long duration gamma-ray burst (GRB) host galaxy detections and upper limits over the redshift range 3<z<5, a key epoch for observational a…

astro-ph.HE2015★ 26 cited

Multiwavelength analysis of three SNe associated with GRBs observed by GROND

F. Olivares E., J. Greiner, P. Schady +14

After the discovery of the first connection between GRBs and SNe almost two decades ago, tens of SN-like rebrightenings have been discovered and about seven solid associations have…

astro-ph.HE2014★ 105 cited

Circular polarization in the optical afterglow of GRB 121024A

K. Wiersema, S. Covino, K. Toma +37

Gamma-ray bursts (GRBs) are most probably powered by collimated relativistic outflows (jets) from accreting black holes at cosmological distances. Bright afterglows are produced wh…

astro-ph.HE2014★ 26 cited

A quiescent galaxy at the position of the long GRB 050219A

A. Rossi, S. Piranomonte, S. Savaglio +25

Long-duration gamma-ray bursts (LGRBs) are produced by the collapse of very massive stars. Due to the short lifetime of their progenitors, LGRBs pinpoint star-forming galaxies. We…

astro-ph.HE2014★ 13 cited

The First Billion Years project: gamma-ray bursts at z>5

J. Elliott, S. Khochfar, J. Greiner +1

Long gamma-ray burst's (LGRB's) association to the death of massive stars suggest they could be used to probe the cosmic star formation history (CSFH) with high accuracy, due to th…

astro-ph.HE2014★ 59 cited

Supernova 2010as: the Lowest-Velocity Member of a Family of Flat-Velocity Type IIb Supernovae

Gastón Folatelli, Melina C. Bersten, Hanindyo Kuncarayakti +23

We present extensive optical and near-infrared photometric and spectroscopic observations of the stripped-envelope (SE) supernova SN 2010as. Spectroscopic peculiarities, such as in…

astro-ph.HE2014★ 33 cited

GROND coverage of the main peak of Gamma-Ray Burst 130925A

J. Greiner, H. -F. Yu, T. Krühler +23

Prompt or early optical emission in gamma-ray bursts is notoriously difficult to measure, and observations of the dozen cases show a large variety of properties. Yet, such early em…

astro-ph.HE2014★ 42 cited

GRB 120711A: an intense INTEGRAL burst with long-lasting soft gamma-ray emission and a powerful optical flash

A. Martin-Carrillo, L. Hanlon, M. Topinka +20

A long and intense gamma-ray burst (GRB) was detected by INTEGRAL on July 11 2012 with a duration of ~115s and fluence of 2.8x10^-4 erg cm^-2 in the 20 keV-8 MeV energy range. GRB…

astro-ph.HE2013

Simultaneous optical/gamma-ray observations of GRB 121217's prompt emission

J. Elliott, H. -F. Yu, S. Schmidl +20

Since the advent of the Swift satellite it has been possible to obtain precise localisations of GRB positions of sub-arcsec accuracy within seconds, facilitating ground-based robot…

astro-ph.HE2013★ 26 cited

Prompt emission of GRB 121217A from gamma-rays to the NIR

J. Elliott, H. -F. Yu, S. Schmidl +20

The mechanism that causes the prompt-emission episode of gamma-ray bursts (GRBs) is still widely debated despite there being thousands of prompt detections. The favoured internal s…

astro-ph.HE2013★ 40 cited

Afterglow rebrightenings as a signature of a long-lasting central engine activity? The emblematic case of GRB 100814A

M. Nardini, J. Elliott, R. Filgas +12

In the past few years the number of well-sampled optical to NIR light curves of long Gamma-Ray Bursts (GRBs) has greatly increased particularly due to simultaneous multi-band image…

astro-ph.HE2013★ 1 cited

The low-extinction afterglow in the solar-metallicity host galaxy of GRB 110918A

J. Elliott, T. Krühler, J. Greiner +21

Galaxies selected through long gamma-ray bursts (GRBs) could be of fundamental importance when mapping the star formation history out to the highest redshifts. Before using them as…

astro-ph.HE2013★ 62 cited

The low-extinction afterglow in the solar-metallicity host galaxy of gamma-ray burst 110918A

J. Elliott, T. Krühler, J. Greiner +21

Metallicity is theoretically thought to be a fundamental driver in gamma-ray burst (GRB) explosions and energetics, but is still, even after more than a decade of extensive studies…

astro-ph.HE2013★ 46 cited

The unusual afterglow of the Gamma-Ray Burst 100621A

J. Greiner, T. Krühler, M. Nardini +27

In order to constrain the broad-band spectral energy distribution of the afterglow of GRB 100621A, dedicated observations were performed in the optical/near-infrared with the 7-cha…

astro-ph.HE2012★ 137 cited

PSR J1311-3430: A Heavyweight Neutron Star with a Flyweight Helium Companion

Roger W. Romani, Alexei V. Filippenko, Jeffery M. Silverman +5

We have obtained initial spectroscopic observations and additional photometry of the newly discovered Pb=94min gamma-ray black-widow pulsar PSR J1311-3430. The Keck spectra show a…

astro-ph.HE2012★ 24 cited

GRB 091029: At the limit of the fireball scenario

R. Filgas, J. Greiner, P. Schady +20

Using high-quality, broad-band afterglow data for GRB 091029, we test the validity of the forward-shock model for gamma-ray burst afterglows. We used multi-wavelength (NIR to X-ray…

astro-ph.HE2012★ 63 cited

Multi-color observations of short GRB afterglows: 20 events observed between 2007 and 2010

A. Nicuesa Guelbenzu, S. Klose, J. Greiner +18

We report on follow-up observations of 20 short-duration gamma-ray bursts performed in g'r'i'z'JHKs with the seven-channel imager GROND between mid-2007 and the end of 2010. This i…

astro-ph.HE2012★ 33 cited

The late-time afterglow of the extremely energetic short burst GRB 090510 revisited

A. Nicuesa Guelbenzu, S. Klose, T. Kruehler +16

The discovery of the short GRB 090510 has raised considerable attention mainly because it had a bright optical afterglow and it is among the most energetic events detected so far w…

astro-ph.HE2011★ 69 cited

The Fast Evolution of SN 2010bh associated with XRF 100316D

Felipe Olivares E., Jochen Greiner, Patricia Schady +13

(...) Since 1998, only half a dozen spectroscopically confirmed associations have been discovered and XRF 100316D associated with the type-Ic SN 2010bh at z = 0.059 is among the la…