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[During its flight ANITA-2 recorded \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${\sim }21.4$$\end{document} million RF triggered events. Simulations of ANITA-2 inform us that the experiment was likely to see very few neutrino-induced signals, with typical estimates in the range \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$O$$\end{document}(0.01–1) events, depending on the neutrino flux model used. Meanwhile, the number of cosmic-rays that triggered ANITA-2 is expected to be lower than the 16 observed by ANITA-1 due to modifications in the trigger scheme used.]
Published: Jul 11, 2012
Keywords: Continuous Wave; Thermal Noise; Interferometric Image; Thermal Background; Minimum Bias Event
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