# ZEU-HESS

 2018-04-2313:37 [PUBDB-2018-01824] Report/Journal Article et al A search for new supernova remnant shells in the Galactic plane with H.E.S.S. [arXiv:1801.06020]   A search for new supernova remnants (SNRs) has been conducted using TeV gamma-ray data from the H.E.S.S. Galactic plane survey. [...] OpenAccess: PDF PDF (PDFA); 2018-03-2614:17 [PUBDB-2018-01567] Report/Journal Article et al H.E.S.S. discovery of very high energy $\gamma$-ray emission from PKS 0625-354 [arXiv:1802.07611] Monthly notices of the Royal Astronomical Society 476(3), 4187 – 4198 (2018) [10.1093/mnras/sty439]   PKS 0625−354 (z = 0.055) was observed with the four High Energy Stereoscopic System (H.E.S.S.) telescopes in 2012 during 5.5 h. The source was detected above an energy threshold of 200 GeV at a significance level of 6.1σ. [...] OpenAccess: PDF PDF (PDFA); 2018-03-1214:01 [PUBDB-2018-01457] Journal Article et al Detection of variable VHE $\gamma$-ray emission from the extra-galactic $\gamma$-ray binary LMC P3   Context.Recently, the high-energy (HE, 0.1–100 GeV) $\gamma$-ray emission from the object LMC P3 in the Large Magellanic Cloud (LMC) has been discovered to be modulated with a 10.3-day period, making it the first extra-galactic $\gamma$-ray binary. Aims. [...] Restricted: PDF PDF (PDFA); 2017-12-0711:00 [PUBDB-2017-12826] Report/Journal Article et al TeV Gamma-Ray Observations of the Binary Neutron Star Merger GW170817 with H.E.S.S. [arXiv:1710.05862] The astrophysical journal / 2 850(2), L22 (2017) [10.3847/2041-8213/aa97d2]   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. [...] Restricted: PDF PDF (PDFA); 2017-11-0214:26 [PUBDB-2017-11668] Dissertation / PhD Thesis et al VHE Gamma-ray sources at the resolution limit of H.E.S.S Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät , 131 pp. (2015) [10.18452/17517] = Humboldt Universität, Dissertation, 2015   Very-high-energy (VHE)γ-ray astronomy deals with the ground-based detection of pho-tons with energies of a few tens of GeV to∼100 TeV by employing the Imaging Air Cherenkov Technique (IACT). This method uses the atmosphere as a detector for VHE γ-rays, exploiting that photons in that energy range produce particle showers by inter-acting with atmospheric particles. [...] OpenAccess: PDF; 2017-10-2714:31 [PUBDB-2017-11596] Dissertation / PhD Thesis Mayer, M. Pulsar wind nebulae at high energies : A diverse population and exceptional twins , 142 pp. (2014) [10.3204/PUBDB-2017-11596] = Universität Potsdam, Dissertation, 2014   Pulsar wind nebulae (PWNe) are the most abundant TeV $\gamma$-ray emitters in the Milky Way. The radiative emission of these objects is powered by fast-rotating pulsars, which donateparts of their rotational energy into winds of relativistic particles. [...] OpenAccess: PDF; 2017-10-2714:26 [PUBDB-2017-11595] Dissertation / PhD Thesis Holler, M. Photon reconstruction for the H.E.S.S. 28 m telescope and analysis of Crab Nebula and Galactic Centre Observations , 86 pp. (2014) = Universität Potsdam, Dissertation, 2014 2017-10-2714:22 [PUBDB-2017-11594] Dissertation / PhD Thesis et al Crab Flare Observationswith H.E.S.S. Phase II , 131 pp. (2014) [10.3204/PUBDB-2017-11594] = Universität Potsdam, Dissertation, 2014   The H.E.S.S. array is a third generation Imaging Atmospheric Cherenkov Telescope (IACT) array. [...] OpenAccess: PDF; 2017-10-2713:13 [PUBDB-2017-11593] Dissertation / PhD Thesis Schulz, A. Search for gamma-ray emission from bow shocks of runaway stars , 138 pp. (2014) [10.3204/PUBDB-2017-11593] = Universität Potsdam, Dissertation, 2014   The mystery of the origin of cosmic rays has been tackled for more than hundred years and is still not solved. Cosmic rays are detected with energies spanning more than 10 orders of magnitude and reaching energies up to ~ 10$^{21}$eV, far higher than any man-made accelerator can reach. [...] OpenAccess: PDF PDF (PDFA); 2017-10-2614:52 [PUBDB-2017-11578] Report/Journal Article et al Measurement of the EBL Spectral Energy Distribution Using the VHE $\gamma$-ray Spectra of H.E.S.S. Blazars [arXiv:1707.06090]   Very high-energy gamma-rays (VHE, E>100 GeV) propagating over cosmological distances can interact with the low-energy photons of the extragalactic background light (EBL) and produce electron-positron pairs. The transparency of the universe to VHE gamma-rays is then directly related to the spectral energy distribution (SED) of the EBL. [...] Restricted: PDF PDF (PDFA);