Cosmic Ray Mass Measurements with LOFAR
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....
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Online Access: | https://doi.org/10.1051/epjconf/201713501009 |
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doaj-5703b33fb59c4d41b1f0f5b3792a4dbd2021-08-02T16:06:45ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011350100910.1051/epjconf/201713501009epjconf_arena2017_01009Cosmic Ray Mass Measurements with LOFARBuitink Stijn0Bonardi Antonio1Corstanje Arthur2Enriquez J. Emilio3Falcke HeinoHörandel Jörg R.Mitra Pragati4Mulrey Katie5Nelles Anna6Rachen Jörg Paul7Rossetto Laura8Schellart Pim9Scholten OlafThoudam Satyendra10Trinh Giater Veen Sander11Winchen Tobias12Vrije Universiteit BrusselDepartment of Astrophysics/IMAPP, Radboud UniversityDepartment of Astrophysics/IMAPP, Radboud UniversityDepartment of Astrophysics/IMAPP, Radboud UniversityVrije Universiteit BrusselVrije Universiteit BrusselUniversity of California IrvineDepartment of Astrophysics/IMAPP, Radboud UniversityDepartment of Astrophysics/IMAPP, Radboud UniversityDepartment of Astrophysics/IMAPP, Radboud UniversityDepartment of Astrophysics/IMAPP, Radboud UniversityAstronVrije Universiteit BrusselIn 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.https://doi.org/10.1051/epjconf/201713501009 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Buitink Stijn Bonardi Antonio Corstanje Arthur Enriquez J. Emilio Falcke Heino Hörandel Jörg R. Mitra Pragati Mulrey Katie Nelles Anna Rachen Jörg Paul Rossetto Laura Schellart Pim Scholten Olaf Thoudam Satyendra Trinh Gia ter Veen Sander Winchen Tobias |
spellingShingle |
Buitink Stijn Bonardi Antonio Corstanje Arthur Enriquez J. Emilio Falcke Heino Hörandel Jörg R. Mitra Pragati Mulrey Katie Nelles Anna Rachen Jörg Paul Rossetto Laura Schellart Pim Scholten Olaf Thoudam Satyendra Trinh Gia ter Veen Sander Winchen Tobias Cosmic Ray Mass Measurements with LOFAR EPJ Web of Conferences |
author_facet |
Buitink Stijn Bonardi Antonio Corstanje Arthur Enriquez J. Emilio Falcke Heino Hörandel Jörg R. Mitra Pragati Mulrey Katie Nelles Anna Rachen Jörg Paul Rossetto Laura Schellart Pim Scholten Olaf Thoudam Satyendra Trinh Gia ter Veen Sander Winchen Tobias |
author_sort |
Buitink Stijn |
title |
Cosmic Ray Mass Measurements with LOFAR |
title_short |
Cosmic Ray Mass Measurements with LOFAR |
title_full |
Cosmic Ray Mass Measurements with LOFAR |
title_fullStr |
Cosmic Ray Mass Measurements with LOFAR |
title_full_unstemmed |
Cosmic Ray Mass Measurements with LOFAR |
title_sort |
cosmic ray mass measurements with lofar |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2017-01-01 |
description |
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. |
url |
https://doi.org/10.1051/epjconf/201713501009 |
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