2016•Proceedings of The 34th International Cosmic Ray Conference — PoS(ICRC2015)Open access

The cosmic-ray energy spectrum above $\sim 10^{16}$ eV measured with the LOFAR Radboud Air Shower Array

S. Thoudam, S. Buitink, A. Corstanje, J. Emilio Enriquez, Heino D. Falcke, J.R. Hörandel, A. Nelles, Jörg Paul Rachen, Laura Rossetto, P. Schellart, Olaf Scholten, Sander Ter Veen, Gia Thi Ngoc Trinh, Luc van Kessel

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Abstract

Figure 1: Schematic layout of the LORA array.Filled squares: LORA detectors, crosses: Low-band antennas, and empty squares: High-band antennas.The dashed circle shows a fiducial region of 150 m radius applied in our analysis.

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What this paper is about

Figure 1: Schematic layout of the LORA array.Filled squares: LORA detectors, crosses: Low-band antennas, and empty squares: High-band antennas.The dashed circle shows a fiducial region of 150 m radius applied in our analysis.

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Available abstract

Figure 1: Schematic layout of the LORA array.Filled squares: LORA detectors, crosses: Low-band antennas, and empty squares: High-band antennas.The dashed circle shows a fiducial region of 150 m radius applied in our analysis.

Key concepts: LOFAR, Physics, Air shower, RADIUS, Detector, Schematic, Astrophysics, Optics

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