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The Surface Enhancement of the IceTop air-shower array will include theaddition of radio antennas and scintillator panels, co-located with theexisting ice-Cherenkov tanks and covering an area of about 1 km$^2$. Together,these will increase the sensitivity of the IceCube Neutrino Observatory to theelectromagnetic and muonic components of cosmic-ray-induced air showers at theSouth Pole. The inclusion of the radio technique necessitates an expanded setof simulation and analysis tools to explore the radio-frequency emission fromair showers in the 70 MHz to 350 MHz band. In this paper we describe thesoftware modules that have been developed to work with time- andfrequency-domain information within IceCube's existing software framework,IceTray, which is used by the entire IceCube collaboration. The softwareincludes a method by which air-shower simulation, generated using CoREAS, canbe reused via waveform interpolation, thus overcoming a significantcomputational hurdle in the field.

Framework and Tools for the Simulation and Analysis of the Radio Emission from Air Showers at IceCube