The Radio Neutrino Observatory Greenland (RNO-G)

S. Wissel, J. Aguilar, P. Allison, J. Beatty, H. Bernhoff, D. Besson, N. Bingefors, O. Botner, S. Bouma, S. Buitink, K. Carter, M. Cataldo, B. Clark, Z. Curtis-Ginsberg, A. Connolly, P. Dasgupta, S. D. Kockere, K. D. Vries, C. Deaconu, M. DuVernois, C. Glaser, A. Hallgren, S. Hallmann, J. Hanson, B. Hendricks, B. Hokanson-Fasig, C. Hornhuber, K. Hughes, A. Karle, J. Kelley, S. Klein, R. Krebs, R. Lahmann, U. Latif, M. Magnuson, T. Meures, Z. Meyers, K. Mulrey, A. Nelles, A. Novikov, E. Oberla, B. Oeyen, H. Pandya, I. Plaisier, L. Pyras, D. Ryckbosch, O. Scholten, D. Seckel, Daniel Smith, D. Southall, J. Torres, S. Toscano, D. Tosi, D. V. D. Broeck, N. Eijndhoven, A. Vieregg, C. Welling, R. Young, A. Zink, Rno-g
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引用次数: 10

Abstract

The Radio Neutrino Observatory Greenland (RNO-G) is scheduled for deployment in the summerof 2021. It will target the detection of astrophysical and cosmogenic neutrinos above 10 PeV. With 35 autonomous stations, it will be the largest implementation of a radio neutrino detector to date.The stations combine best-practice instrumentation from all previous radio neutrino arrays, such as a deep phased-array trigger and surface antennas. These proceedings describe the experimentalconsiderations that have driven the design of RNO-G and the current progress in deployment, aswell as discuss the projected sensitivity of the instrument. RNO-G will provide a unique view ofthe Northern Sky and will also inform the design of the radio component of IceCube-Gen2.
格陵兰射电中微子天文台(RNO-G)
格陵兰射电中微子天文台(RNO-G)计划于2021年夏天部署。它的目标是探测10 PeV以上的天体物理和宇宙中微子。它拥有35个独立的观测站,将是迄今为止最大的射电中微子探测器。这些观测站结合了以前所有射电中微子阵列的最佳实践仪器,如深相控阵触发器和表面天线。这些程序描述了驱动RNO-G设计的实验考虑因素和部署的当前进展,并讨论了仪器的预计灵敏度。RNO-G将提供一个独特的北方天空视图,也将为冰立方- gen2的无线电组件的设计提供信息。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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