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  1. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference)
    Free, publicly-accessible full text available January 1, 2023
  2. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference.)
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  3. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference)
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  4. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference.)
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  5. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference)
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  6. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference.)
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  7. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference)
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  8. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference.)
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  9. ; ; ; ; ; ; ; ; ; ; et al ( , Journal of Instrumentation)
    Abstract The Surface Enhancement of the IceTop air-shower array will include the addition of radio antennas and scintillator panels, co-located with the existing ice-Cherenkov tanks and covering an area of about 1 km 2 . Together, these will increase the sensitivity of the IceCube Neutrino Observatory to the electromagnetic and muonic components of cosmic-ray-induced air showers at the South Pole. The inclusion of the radio technique necessitates an expanded set of simulation and analysis tools to explore the radio-frequency emission from air showers in the 70 MHz to 350 MHz band. In this paper we describe the software modules thatmore »have been developed to work with time- and frequency-domain information within IceCube's existing software framework, IceTray, which is used by the entire IceCube collaboration. The software includes a method by which air-shower simulation, generated using CoREAS, can be reused via waveform interpolation, thus overcoming a significant computational hurdle in the field.« less
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  10. ; ; ; ; ; ; ; ; ; ; et al ( , Physical Review Letters)
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