activity
20092026
most citedPerformance of two Askaryan Radio Array stations and first results in the search for ultra-high energy neutrinos

144 citations · 559 across the 23 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

12 papers · 1 filter

astro-ph.IM2026

Trigger system for the Payload for Ultrahigh Energy Observations (PUEO) balloon-borne neutrino detector

Q. Abarr, J. Alfaro, P. Allison +67

The Payload for Ultrahigh Energy Observations (PUEO) is a NASA balloon-borne instrument for the detection of ultra-high energy (UHE) neutrinos with energies above $10^{17.5}~\textr…

astro-ph.IM2024★ 1 cited

Modeling the refractive index profile n(z) of polar ice for ultra-high energy neutrino experiments

S. Ali, P. Allison, S. Archambault +67

We have developed an in-situ index of refraction profile n(z) for cold polar ice, using the transit times of radio signals broadcast from an englacial transmitter to 2-5 km distant…

astro-ph.IM2023

Calibration and Physics with ARA Station 1: A Unique Askaryan Radio Array Detector

M. F. H Seikh, D. Z. Besson, S. Ali +70

The Askaryan Radio Array Station 1 (A1), the first among five autonomous stations deployed for the ARA experiment at the South Pole, is a unique ultra-high energy neutrino (UHEN) d…

astro-ph.IM2021★ 11 cited

The SLAC T-510 experiment for radio emission from particle showers: detailed simulation study and interpretation

K. Bechtol, K. Belov, K. Borch +26

Over the last several decades, radio detection of air showers has been widely used to detect ultra-high-energy cosmic rays. We developed an experiment under controlled laboratory c…

astro-ph.IM2021★ 6 cited

Triboelectric Backgrounds to radio-based UHE Neutrino Exeperiments

J. A. Aguilar, A. Anker, P. Allison +114

The proposed IceCube-Gen2 (ICG2) seeks to instrument ~500 sq. km of Antarctic ice near the geographic South Pole with radio antennas, in order to observe the highest energy (E>1 Ee…

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…

astro-ph.IM2017★ 10 cited

Dynamic tunable notch filters for the Antarctic Impulsive Transient Antenna (ANITA)

P. Allison, O. Banerjee, J. J. Beatty +56

The Antarctic Impulsive Transient Antenna (ANITA) is a NASA long-duration balloon experiment with the primary goal of detecting ultra-high-energy ($>10^{18}\,\mbox{eV}$) neutrinos…

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.IM2015★ 49 cited

Accelerator measurements of magnetically-induced radio emission from particle cascades with applications to cosmic-ray air showers

K. Belov, K. Mulrey, A. Romero-Wolf +25

For fifty years, cosmic-ray air showers have been detected by their radio emission. We present the first laboratory measurements that validate electrodynamics simulations used in a…

astro-ph.IM2012★ 4 cited

A next generation Ultra-Fast Flash Observatory (UFFO-100) for IR/optical observations of the rise phase of gamma-ray bursts

B. Grossan, I. H. Park, S. Ahmad +39

The Swift Gamma-ray Burst (GRB) observatory responds to GRB triggers with optical observations in ~ 100 s, but cannot respond faster than ~ 60 s. While some ground-based telescopes…

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…