Cosmic Ray Mass Measurements with LOFAR
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ID: 99528
2017
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Abstract
In the dense core of LOFAR individual air showers are detected by hundreds of dipole antennas simultaneously. We reconstruct Xmax by using a hybrid technique that combines a two-dimensional fit of the radio profile to CoREAS simulations and a one-dimensional fit of the particle density distribution. For high-quality detections, the statistical uncertainty on Xmax is smaller than 20 g/cm2. We present results of cosmic-ray mass analysis in the energy regime of 1017 - 1017.5 eV. This range is of particular interest as it may harbor the transition from a Galactic to an extragalactic origin of cosmic rays.
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stijn2017cosmicepj
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| Authors | Stijn, Buitink;Antonio, Bonardi;Arthur, Corstanje;Emilio, Enriquez J.;Heino, Falcke;R., Hörandel Jörg;Pragati, Mitra;Katie, Mulrey;Anna, Nelles;Paul, Rachen Jörg;Laura, Rossetto;Pim, Schellart;Olaf, Scholten;Satyendra, Thoudam;Gia, Trinh;Sander, ter Veen;Tobias, Winchen; |
| Journal | epj web of conferences |
| Year | 2017 |
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