Add to ORKGAbstract: AraSim is a software package used by the Askaryan Radio Array (ARA) collaboration to simulate the detector response to radio Cherenkov emission from ultra-high energy (UHE) neutrino interactions. We provide details of simulated neutrino events in AraSim, including neutrino absorption in the Earth, the radio Cherenkov signal spectrum, determining the signal’s propagation through the Antarctic ice, and modeling properties of the detector. We also present the results of calibrating AraSim to TestBed data and the expected UHE neutrino sensitivity of data from different deployment stages of ARA detector
The Askar'yan Radio Array (ARA), a neutrino detector to be situated at the South Pole next to the Ic...
GZK neutrino are interesting messenger particles since, if detected, they can transmit<p>us exclusiv...
The Askar'yan Radio Array (ARA), a neutrino detector to be situated at the South Pole, will be sensi...
Abstract: The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) cosmic neutrino detector loca...
Abstract The Askaryan Radio Array (ARA) is an ultra-high energy (>1017 eV) cosmic neutrino detector ...
The Askaryan Radio Array (ARA) is an experiment looking for the Askaryan emission of cosmogenic neut...
Abstract: We describe the physics goals and detector capabilities of the the ARIANNA High Energy Neu...
Ultrahigh energy neutrinos are interesting messenger particles since, if detected, they can transmit...
Abstract: A new generation of neutrino telescopes is being established with the use of low noise, lo...
Abstract: The third flight of the high-altitude balloon-borne ANtarctic Impulsive Transient Antenna ...
To observe high energy cosmogenic neutrinos above 50 PeV, the large neutrino telescope ARA is being ...
We report on studies of the viability and sensitivity of the Askaryan Radio Array (ARA), a new initi...
Detecting astrophysical neutrinos at the highest known energies will help answer critically importan...
The ARIANNA pilot Hexagonal Radio Array (HRA), a seven station test-bed for the development of an ul...
The emerging field of radio based neutrino astronomy holds promise in answering long lasting questio...
The Askar'yan Radio Array (ARA), a neutrino detector to be situated at the South Pole next to the Ic...
GZK neutrino are interesting messenger particles since, if detected, they can transmit<p>us exclusiv...
The Askar'yan Radio Array (ARA), a neutrino detector to be situated at the South Pole, will be sensi...
Abstract: The Askaryan Radio Array (ARA) is an ultra-high energy (UHE) cosmic neutrino detector loca...
Abstract The Askaryan Radio Array (ARA) is an ultra-high energy (>1017 eV) cosmic neutrino detector ...
The Askaryan Radio Array (ARA) is an experiment looking for the Askaryan emission of cosmogenic neut...
Abstract: We describe the physics goals and detector capabilities of the the ARIANNA High Energy Neu...
Ultrahigh energy neutrinos are interesting messenger particles since, if detected, they can transmit...
Abstract: A new generation of neutrino telescopes is being established with the use of low noise, lo...
Abstract: The third flight of the high-altitude balloon-borne ANtarctic Impulsive Transient Antenna ...
To observe high energy cosmogenic neutrinos above 50 PeV, the large neutrino telescope ARA is being ...
We report on studies of the viability and sensitivity of the Askaryan Radio Array (ARA), a new initi...
Detecting astrophysical neutrinos at the highest known energies will help answer critically importan...
The ARIANNA pilot Hexagonal Radio Array (HRA), a seven station test-bed for the development of an ul...
The emerging field of radio based neutrino astronomy holds promise in answering long lasting questio...
The Askar'yan Radio Array (ARA), a neutrino detector to be situated at the South Pole next to the Ic...
GZK neutrino are interesting messenger particles since, if detected, they can transmit<p>us exclusiv...
The Askar'yan Radio Array (ARA), a neutrino detector to be situated at the South Pole, will be sensi...