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  • Miocinovic, P; Barwick, S. W; Beatty, J. J; Besson, D. Z; Binns, W. R; Cai, B; Clem, J. M; Connolly, A; Coutu, S; Cowen, D. F; Dowkontt, P. F; DuVernois, M. A; Evenson, P. A; Goldstein, D; Gorham, P. W; Hebert, C. L; Israel, M. H; Learned, J. G; Liewer, K. M; Link, J. T; Matsuno, S; Nam, J. W; Naudet, C. J; Nichol, R; Palladino, K. J; Rosen, M; Saltzberg, D; Seckel, D; Silvestri, A; Varner, G. S; Williams, D

    arXiv (Cornell University), 03/2005
    Journal Article

    ECONF C041213:2516,2004 The Antarctic Impulsive Transient Antenna (ANITA) experiment is being developed to search for ultra-high-energy (UHE) neutrino interactions ($>3\times10^{18}$ eV) in the Antarctic ice cap. A neutrino interaction in the ice will produce a radio pulse by the means of the Askaryan effect. The large radio transparency of ice allows for such a pulse to be recorded by a cluster of balloon-borne antennas. The details of the ANITA instrument, now in a construction phase, and the science we hope to achieve is discussed. In order to prepare for the main mission, we have flown ANITA-lite during the 2003/04 austral season. ANITA-lite consisted of two quad-ridge horn antennas and a prototype RF (radio frequency) triggering and recording system. Here we present the results of an impulsive RF background survey of Antarctica, as well as proof-of-principle gain, tracking, and timing calibrations conducted by observing solar radio emissions and calibration radio-pulses. A preliminary UHE neutrino flux limit based on ANITA-lite data is also presented.