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Unraveling The Complex Nature Of The Very High-Energy -Ray Blazar PKS 2155-304
Alicja Wierzcholska, Michael Zacharias, Felix Jankowsky +2
PKS 2155-304 is a blazar located in the Southern Hemisphere, monitored with the High Energy Stereoscopic System (H.E.S.S.) at very high energy (VHE, E>100 GeV) rays every year…
News from the very-high-energy sky seen with H.E.S.S
Andreas Zech, H. E. S. S. Collaboration
The H.E.S.S. experiment, the largest Cherenkov telescope array to date, has been observing the sky at TeV energies for the past 16 years. Its location in the Southern hemisphere pr…
Resolving the Crab pulsar wind nebula at teraelectronvolt energies
H. E. S. S. Collaboration, H. Abdalla, F. Aharonian +221
The Crab nebula is one of the most studied cosmic particle accelerators, shining brightly across the entire electromagnetic spectrum up to very high-energy gamma rays. It is known…
Dark Matter search with H.E.S.S. towards ultra-faint dwarf nearby DES satellites of the Milky Way
Lucia Rinchiuso, Emmanuel Moulin, Céline Armand +2
Several nearby ultra-faint satellites of the Milky Way discovered by the Dark Energy Survey (DES) during the last few years are promising targets for indirect dark matter (DM) sear…
Search for Point-Like TeV Sources in the Large Magellanic Cloud
Nukri Komin, Maria Haupt, H. E. S. S. Collaboration
The Large Magellanic Cloud (LMC) is an irregular satellite galaxy of the Milky Way, which has been observed extensively in Very-High-Energy (VHE) gamma rays with the H.E.S.S. teles…
Constraints on the emission region of 3C 279 during strong flares in 2014 and 2015 through VHE gamma-ray observations with H.E.S.S
H. E. S. S. Collaboration, H. Abdalla, R. Adam +224
The flat spectrum radio quasar 3C 279 is known to exhibit pronounced variability in the high-energy (MeVGeV) -ray band, which is continuously monitored with Fer…