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L. Stawarz

Researcher at Max Planck Society

Publications -  9
Citations -  2012

L. Stawarz is an academic researcher from Max Planck Society. The author has contributed to research in topics: High Energy Stereoscopic System & Crab Nebula. The author has an hindex of 9, co-authored 9 publications receiving 1924 citations.

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Energy Spectrum of Cosmic-Ray Electrons at TeV Energies

Felix Aharonian, +155 more
TL;DR: In this measurement, the first of this type, the High Energy Stereoscopic System is able to extend the measurement of the electron spectrum beyond the range accessible to direct measurements, finding evidence for a substantial steepening in the energy spectrum above 600 GeV compared to lower energies.
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Probing the ATIC peak in the cosmic-ray electron spectrum with H.E.S.S.

Felix Aharonian, +168 more
TL;DR: In this article, the authors present a measurement of the cosmic-ray electron spectrum with H.E.S. starting at 340 GeV and show no indication of a structure in the electron spectrum, but rather a power-law spectrum with spectral index of 3.0 +- 0.1 (stat.) + − 0.3 (syst.) which steepens at about 1 TeV.
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New constraints on the mid-IR EBL from the HESS discovery of VHE gamma-rays from 1ES 0229+200

Felix Aharonian, +143 more
TL;DR: In this paper, a very high energy (VHE: >100 GeV) γ-ray emission from the high-frequency peaked BL Lac 1ES 0229+200 was detected at the 6.6σ level in the HESS observations (41.8 h live time).
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HESS very-high-energy gamma-ray sources without identified counterparts

Felix Aharonian, +143 more
TL;DR: In this article, the authors investigated the very high-energy (VHE) gamma-ray sources that have been discovered with HESS in the most sensitive blind survey of the Galactic plane at VHE energies conducted so far.
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Discovery of VHE gamma-rays from the distant BL Lacertae 1ES 0347-121

Felix Aharonian, +143 more
TL;DR: In this paper, the authors used the observed VHE spectrum to derive limits on the Extragalactic Background Light (EBL) and determined physical quantities through the modeling of the object's broad-band spectral energy distribution (SED).