Progress Towards a Diffuse Neutrino Search in the Full Livetime of the Askaryan Radio Array
Paramita Dasgupta, Marco Stein Muzio (for the ARA Collaboration)

TL;DR
This paper reports on a comprehensive search for ultra-high-energy neutrinos using the full data set of the Askaryan Radio Array, highlighting improved analysis techniques and expected to set leading limits above 100 PeV.
Contribution
It introduces a full-livetime neutrino search with the ARA, combining multiple stations and advanced analysis methods to enhance detection capabilities and background rejection.
Findings
Anticipated to set world-leading limits above 100 PeV.
Demonstrates improved analysis efficiencies and background rejection.
Integrates data from all five stations for a comprehensive search.
Abstract
The Askaryan Radio Array (ARA) is an in-ice ultrahigh energy (UHE, PeV) neutrino experiment at the South Pole that aims to detect radio emissions from neutrino-induced particle cascades. ARA has five independent stations which together have collected nearly 24 station-years of data. Each of these stations search for UHE neutrinos by burying in-ice clusters of antennas m deep in a roughly cubical lattice with side length m. Additionally, the fifth ARA station (A5) has a beamforming trigger, referred to as the Phased Array (PA), consisting of a trigger array of 7 tightly packed vertically-polarized antennas. In this proceeding, we will present a neutrino search with the data of this "hybrid" station, emphasizing its capabilities for improved analysis efficiencies, background rejection, and neutrino vertex reconstruction. This is enabled by combining the closely…
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