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Showing 1 to 4 of 4 for “"Gammastrahlungsastronomie"”.

  1. Crab flare observations with H.E.S.S. phase II

    The H.E.S.S. array is a third generation Imaging Atmospheric Cherenkov Telescope (IACT) array. It is located in the Khomas Highland in Namibia, and measures very high energy (VHE) gamma-rays. In Phase I, the array started data taking in 2004 with its four identical 13 m telescopes. Since then, …

    potsdam-diss Repository record for Crab flare observations with H.E.S.S. phase II (opens in a new tab)

  2. Search for gamma-ray emission from bow shocks of runaway stars

    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 ~10²¹ eV, far higher than any man-made accelerator can reach. Different …

    potsdam-diss Repository record for Search for gamma-ray emission from bow shocks of runaway stars (opens in a new tab)

  3. Photon reconstruction for the H.E.S.S. 28 m telescope and analysis of Crab Nebula and galactic centre observations

    In the presented thesis, the most advanced photon reconstruction technique of ground-based γ-ray astronomy is adapted to the H.E.S.S. 28 m telescope. The method is based on a semi-analytical model of electromagnetic particle showers in the atmosphere. The properties of cosmic γ-rays are …

    potsdam-diss Repository record for Photon reconstruction for the H.E.S.S. 28 m telescope and analysis of Crab Nebula and galactic centre observations (opens in a new tab)

  4. Pulsar wind nebulae at high energies

    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 donate parts of their rotational energy into winds of relativistic particles. This thesis presents an in-depth study of the …

    potsdam-diss Repository record for Pulsar wind nebulae at high energies (opens in a new tab)