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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Main Authors: 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
Format: Article
Language:English
Published: EDP Sciences 2017-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201713501009
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spelling 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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