activity
20052024
most citedNo supernovae associated with two long-duration gamma ray bursts

447 citations · 3k across the 35 of their papers we have counts for

collaborators

35 papers

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.HE2019★ 22 cited

The late-time afterglow evolution of long gamma-ray bursts GRB 160625B and GRB 160509A

Tuomas Kangas, Andrew S. Fruchter, S. Bradley Cenko +12

We present post-jet-break \textit{HST}, VLA and \textit{Chandra} observations of the afterglow of the long -ray bursts GRB 160625B (between 69 and 209 days) and GRB 160509A (bet…

astro-ph.GA2019★ 4 cited

Supernovae SDSS Host Metallicity Catalog and Resulting Metallicity Distributions by SNe Type

John F. Graham

In support of ongoing projects we have compiled a database of supernovae with host metallicities determined from spectroscopy in the Sloan Digital Sky Survey (SDSS) which we are pr…

astro-ph.HE2019★ 4 cited

A Surprising Lack of Metallicity Evolution with Redshift in the Long Gamma-Ray Burst Host Galaxy Population

J. F. Graham, P. Schady, A. S. Fruchter

The number of long-duration Gamma Ray Burst (LGRB) host galaxies with measured metallicities and host masses has now grown to over one hundred, allowing us to investigate how the d…

astro-ph.HE2018★ 14 cited

GRB 151027B - large-amplitude late-time radio variability

J. Greiner, J. Bolmer, M. Wieringa +20

Deriving physical parameters from gamma-ray burst afterglow observations remains a challenge, even now, 20 years after the discovery of afterglows. The main reason for the lack of…

astro-ph.GA2017★ 42 cited

The environment of the SN-less GRB 111005A at z = 0.0133

M. Tanga, T. Krühler, P. Schady +5

The collapsar model has proved highly successful in explaining the properties of long gamma-ray bursts (GRBs), with the most direct confirmation being the detection of a supernova…