Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Neutrino. NU-astrophysical neutrinos
M.Y. Lu,* C.G. Pfendner, A. Shultz on behalf of the ARA Collaboration
*corresponding author
Full text: pdf
Pre-published on: August 16, 2017
Published on: August 03, 2018
Abstract
The Askaryan Radio Array (ARA) is an ultra-high energy neutrino telescope aiming to discover and determine the cosmic neutrino flux above $\sim$100PeV. Under phased construction near the South Pole, ARA achieves the sensitivity through the detection of Askaryan emissions from neutrino-induced showers in the Antarctic ice using radio frequency antennas (150-850MHz). Two ARA stations at a design depth of 200m have been deployed since 2013. We present in this contribution various neutrino search methods developed, and the search results using data from 2013 and after.
DOI: https://doi.org/10.22323/1.301.0966
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