activity
20112019
most citedPerformance of two Askaryan Radio Array stations and first results in the search for ultra-high energy neutrinos

144 citations · 581 across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2019★ 2 cited

Recent Results from The Askaryan Radio Array

ARA Collaboration, P. Allison, S. Archambault +61

The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) neutrino telescope at the South Pole consisting of an array of radio antennas aimed at detecting the Askaryan radiation…

astro-ph.HE2018★ 2 cited

Observation of Reconstructable Radio Emission Coincident with an X-Class Solar Flare in the Askaryan Radio Array Prototype Station

P. Allison, S. Archambault, J. Auffenberg +74

The Askaryan Radio Array (ARA) reports an observation of radio emission coincident with the "Valentine's Day" solar flare on Feb. 15, 2011 in the prototype "Testbed" st…

astro-ph.IM2018★ 14 cited

Antarctic Surface Reflectivity Calculations and Measurements from the ANITA-4 and HiCal-2 Experiments

S. Prohira, A. Novikov, P. Dasgupta +54

The balloon-borne HiCal radio-frequency (RF) transmitter, in concert with the ANITA radio-frequency receiver array, is designed to measure the Antarctic surface reflectivity in the…

astro-ph.IM2017★ 2 cited

Measurement of the real dielectric permittivity epsilon_r of glacial ice

P. Allison, S. Archambault, J. Auffenberg +66

Using data collected by the Askaryan Radio Array (ARA) experiment at the South Pole, we have used long-baseline propagation of radio-frequency signals to extract information on the…

physics.ins-det2017★ 16 cited

HiCal 2: An instrument designed for calibration of the ANITA experiment and for Antarctic surface reflectivity measurements

S. Prohira, A. Novikov, D. Z. Besson +55

The NASA supported High-Altitude Calibration (HiCal)-2 instrument flew as a companion balloon to the ANITA-4 experiment in December 2016. Based on a HV discharge pulser producing r…

astro-ph.IM2017★ 7 cited

Implementation of a custom time-domain firmware trigger for RADAR-based cosmic ray detection

S Prohira, D Besson, S Kunwar +2

Interest in Radio-based detection schemes for ultra-high energy cosmic rays (UHECR) has surged in recent years, owing to the potentially very low cost/detection ratio. The method o…

astro-ph.IM2017

Antarctic Surface Reflectivity Measurements from the ANITA-3 and HiCal-1 Experiments

P. W. Gorham, P. Allison, O. Banerjee +53

The primary science goal of the NASA-sponsored ANITA project is measurement of ultra-high energy neutrinos and cosmic rays, observed via radio-frequency signals resulting from a ne…

astro-ph.HE2015★ 144 cited

Performance of two Askaryan Radio Array stations and first results in the search for ultra-high energy neutrinos

ARA Collaboration, P. Allison, R. Bard +64

Ultra-high energy neutrinos are interesting messenger particles since, if detected, they can transmit exclusive information about ultra-high energy processes in the Universe. These…

astro-ph.HE2015★ 8 cited

Constraints on the Ultra-High Energy Neutrino Flux from Gamma-Ray Bursts from a Prototype Station of the Askaryan Radio Array

P. Allison, J. Auffenberg, R. Bard +49

We report on a search for ultra-high-energy (UHE) neutrinos from gamma-ray bursts (GRBs) in the data set collected by the Testbed station of the Askaryan Radio Array (ARA) in 2011…

astro-ph.IM2015★ 15 cited

Design, Construction and Operation of a Low-Power, Autonomous Radio-Frequency Data-Acquisition Station for the TARA Experiment

S. Kunwar, R. Abbasi, C. Allen +19

Employing a 40-kW radio-frequency transmitter just west of Delta, UT, and operating at 54.1 MHz, the TARA (Telescope Array RAdar) experiment seeks radar detection of extensive air…

astro-ph.IM2014★ 23 cited

Design and Performance of the ARIANNA Hexagonal Radio Array Systems

S. W. Barwick, E. C. Berg, D. Z. Besson +16

We report on the development, installation and operation of the first three of seven stations deployed at the ARIANNA site's pilot Hexagonal Radio Array in Antarctica. The primary…

astro-ph.HE2014★ 133 cited

A First Search for Cosmogenic Neutrinos with the ARIANNA Hexagonal Radio Array

ARIANNA Collaboration, S. W. Barwick, E. C. Berg +35

The ARIANNA experiment seeks to observe the diffuse flux of neutrinos in the 10^8 - 10^10 GeV energy range using a grid of radio detectors at the surface of the Ross Ice Shelf of A…

astro-ph.IM2014★ 34 cited

Time Domain Response of the ARIANNA Detector

S. W. Barwick, E. C. Berg, D. Z. Besson +12

The Antarctic Ross Ice Shelf Antenna Neutrino Array (ARIANNA) is a high-energy neutrino detector designed to record the Askaryan electric field signature of cosmogenic neutrino int…

astro-ph.IM2014★ 22 cited

Telescope Array Radar (TARA) Observatory for Ultra-High Energy Cosmic Rays

R. Abbasi, M. Abou Bakr Othman, C. Allen +19

Construction was completed during summer 2013 on the Telescope Array RAdar (TARA) bi-static radar observatory for Ultra-High Energy Cosmic Rays (UHECR). TARA is co-located with the…

astro-ph.HE2014★ 77 cited

First Constraints on the Ultra-High Energy Neutrino Flux from a Prototype Station of the Askaryan Radio Array

ARA Collaboration, P. Allison, J. Auffenberg +48

The Askaryan Radio Array (ARA) is an ultra-high energy ( eV) cosmic neutrino detector in phased construction near the South Pole. ARA searches for radio Cherenkov emissio…

physics.ins-det2014★ 3 cited

Design, Modeling and Testing of the Askaryan Radio Array South Pole Autonomous Renewable Power Stations

D. Z. Besson, D. M. Kennedy, K. Ratzlaff +1

We describe the design, construction and operation of the Askaryan Radio Array (ARA) Autonomous Renewable Power Stations, initially installed at the South Pole in December, 2010 wi…

astro-ph.HE2011★ 79 cited

Updated Results from the RICE Experiment and Future Prospects for Ultra-High Energy Neutrino Detection at the South Pole

Ilya Kravchenko, Dave Seckel, Dave Besson +4

The RICE experiment seeks observation of ultra-high energy (UHE; >100 PeV) neutrinos interacting in Antarctic ice, by measurement of the radiowavelength Cherenkov radiation resulti…

astro-ph.IM2011

Design and Initial Performance of the Askaryan Radio Array Prototype EeV Neutrino Detector at the South Pole

P. Allison, J. Auffenberg, R. Bard +45

We report on studies of the viability and sensitivity of the Askaryan Radio Array (ARA), a new initiative to develop a Teraton-scale ultra-high energy neutrino detector in deep, ra…