output
20052025
most citedObservations of the Crab Nebula with H.E.S.S

863 citations

Showing 2017Show all

17 papers · 1 filter

astro-ph.HE201764 cited

TeV gamma-ray observations of the binary neutron star merger GW170817 with H.E.S.S

H. E. S. S. Collaboration, :, H. Abdalla +250

We search for high-energy gamma-ray emission from the binary neutron star merger GW170817 with the H.E.S.S. Imaging Air Cherenkov Telescopes. The observations presented here have b…

astro-ph.HE201734 cited

Cloud ablation by a relativistic jet and the extended flare in CTA 102 in 2016 and 2017

M. Zacharias, M. Böttcher, F. Jankowsky +3

In late 2016 and early 2017 the flat spectrum radio quasar CTA 102 exhibited a very strong and long-lasting outburst. The event can be described by a roughly 2 months long increase…

astro-ph.HE20172 cited

Hard X-ray Quiescent Emission in Magnetars via Resonant Compton Upscattering

M. G. Baring, Z. Wadiasingh, P. L. Gonthier +1

Non-thermal quiescent X-ray emission extending between 10 keV and around 150 keV has been seen in about 10 magnetars by RXTE, INTEGRAL, Suzaku, NuSTAR and Fermi-GBM. For inner magn…

physics.plasm-ph20171 cited

Simulating the Injection of Magnetized Plasma without Electromagnetic Precursor Wave

Patrick Kilian, Felix Spanier

Injecting magnetized plasma with changes in magnetization or injection rate necessitate a time variable magnetic field at the boundary of the simulation box. Naive implementation w…

astro-ph.SR201716 cited

Whole Earth Telescope discovery of a strongly distorted quadrupole pulsation in the largest amplitude rapidly oscillating Ap star

Daniel L. Holdsworth, Donald W. Kurtz, Hideyuki Saio +7

We present a new analysis of the rapidly oscillating Ap (roAp) star, 2MASS J (J1940; ). The star was discovered using SuperWASP broadband photometry to ha…

astro-ph.HE20179 cited

Identifying the brightest Galactic globular clusters for future observations by H.E.S.S. and CTA

Hambeleleni Ndiyavala, Petrus Paulus Kruger, Christo Venter

We present results from an emission code that assumes millisecond pulsars (MSPs) to be sources of relativistic particles in globular clusters (GCs) and models the resulting spectra…