output
20052015
most citedObservations of the Crab Nebula with H.E.S.S

863 citations

Showing 2014 · astro-ph.HEShow all

7 papers · 2 filters

astro-ph.HE201430 cited

H.E.S.S. detection of TeV emission from the interaction region between the supernova remnant G349.7+0.2 and a molecular cloud

H. E. S. S. Collaboration, :, A. Abramowski +224

G349.7+0.2 is a young Galactic supernova remnant (SNR) located at the distance of 11.5 kpc and observed across the entire electromagnetic spectrum from radio to high energy (HE) Ga…

astro-ph.HE2014

Modelling the -ray and radio light curves of the double pulsar system

A. S. Seyffert, C. Venter, A. K. Harding +1

Guillemot et al. recently reported the discovery of -ray pulsations from the 22.7ms pulsar (pulsar A) in the famous double pulsar system J0737-3039A/B. The -ray light curve (…

astro-ph.HE20142 cited

Probing cluster environments of blazars through gamma-gamma absorption

Iurii Sushch, Markus Böttcher

Most blazars are known to be hosted in giant elliptic galaxies, but their cluster environments have not been thoroughly investigated. Cluster environments may contain radiation fie…

astro-ph.HE201433 cited

The high-energy -ray emission of AP Librae

H. E. S. S. Collaboration, Fermi-LAT collaborations

The -ray spectrum of the low-frequency-peaked BL Lac (LBL) object AP Librae is studied, following the discovery of very-high-energy (VHE; ) -ray emission up…

astro-ph.HE201441 cited

A self-consistent and time-dependent hybrid blazar emission model - Properties and application

Matthias Weidinger, Felix Spanier

A time-dependent emission model for blazar jets, taking acceleration due to Fermi-I and Fermi-II processes for electrons and protons as well as all relevant radiative processes sel…

astro-ph.HE2014112 cited

Search for dark matter annihilation signatures in H.E.S.S. observations of Dwarf Spheroidal Galaxies

H. E. S. S. Collaboration, :, A. Abramowski +229

Dwarf spheroidal galaxies of the Local Group are close satellites of the Milky Way characterized by a large mass-to-light ratio and are not expected to be the site of non-thermal h…