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Reconstruction of very inclined air showers with radio data and application to the first GRANDProto300 cosmic-ray candidates
Radio detection of very inclined extensive air showers (EAS) offers a promising way to study ultra-high-energy cosmic rays (UHECRs) and neutrinos above $10^{17}$ eV. We present a method to reconstruct the arrival direction and energy of EAS with zenith angles above $60^\circ$, applicable in principl
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