activity
20152024
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 3.6k across the 36 of their papers we have counts for

collaborators

37 papers

astro-ph.HE2024★ 1 cited

Origin of the strong sodium absorption of the lensed supernova 2016geu at z=0.4

Christa Gall, Jens Hjorth, Lise Christensen +7

The origin of strong sodium absorption, which has been observed for a few nearby Type Ia supernovae (SNe Ia), remains elusive. Here we analyse two high-signal-to-noise, intermediat…

astro-ph.HE2021

GRB 160410A: the first Chemical Study of the Interstellar Medium of a Short GRB

J. F. Agüí Fernández, C. C. Thöne, D. A. Kann +27

Short Gamma-Ray Bursts (SGRBs) are produced by the coalescence of compact binary systems which are remnants of massive stars. GRB 160410A is classified as a short-duration GRB with…

astro-ph.HE2020★ 226 cited

Observation of inverse Compton emission from a long -ray burst

V. A. Acciari, S. Ansoldi, L. A. Antonelli +301

Long-duration gamma-ray bursts (GRBs) originate from ultra-relativistic jets launched from the collapsing cores of dying massive stars. They are characterised by an initial phase o…

astro-ph.HE2020★ 59 cited

An Unambiguous Separation of Gamma-Ray Bursts into Two Classes from Prompt Emission Alone

Christian K. Jespersen, Johann B. Severin, Charles L. Steinhardt +4

The duration of a gamma-ray burst (GRB) is a key indicator of its physics origin, with long bursts perhaps associated with the collapse of massive stars and short bursts with merge…

astro-ph.GA2019★ 44 cited

X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at

Mikkel Stockmann, Sune Toft, Anna Gallazzi +23

We present a detailed analysis of a large sample of spectroscopically confirmed ultra-massive quiescent galaxies () at . This sam…

astro-ph.HE2019★ 4 cited

GRB 190114C in the nuclear region of an interacting galaxy -- A detailed host analysis using ALMA, HST and VLT

A. de Ugarte Postigo, C. C. Thöne, S. Martın +28

GRB 190114C is the first GRB for which the detection of very-high energy emission up to the TeV range has been reported. It is still unclear whether environmental properties might…