Andrew Zeolla
YOU?
Author Swipe
View article: The Hybrid Elevated Radio Observatory for Neutrinos (HERON) Project
The Hybrid Elevated Radio Observatory for Neutrinos (HERON) Project Open
View article: Detection of Cosmic Rays at High Elevation by the BEACON Prototype
Detection of Cosmic Rays at High Elevation by the BEACON Prototype Open
View article: The Payload for Ultrahigh Energy Observations: Detector Design and Implementation
The Payload for Ultrahigh Energy Observations: Detector Design and Implementation Open
View article: Searching for Ultrahigh Energy Neutrinos with PUEO
Searching for Ultrahigh Energy Neutrinos with PUEO Open
View article: Optimizing HERON for 100 PeV Neutrino Detection
Optimizing HERON for 100 PeV Neutrino Detection Open
View article: Optimizing HERON for 100 PeV Neutrino Detection
Optimizing HERON for 100 PeV Neutrino Detection Open
The Hybrid Elevated Radio Observatory for Neutrinos (HERON) is designed to target the astrophysical flux of Earth-skimming tau neutrinos at 100 PeV. HERON consists of multiple compact, phased radio arrays embedded within a larger sparse ar…
View article: Sensitivity of BEACON to ultra-high energy diffuse and transient neutrinos
Sensitivity of BEACON to ultra-high energy diffuse and transient neutrinos Open
Ultra-high energy neutrinos ( E > 10 17 eV) can provide insight into the most powerful accelerators in the universe, however their flux is extremely low. The Beamforming Elevated Array for COsmic Neutrinos (BEACON) is a detector concept wh…
View article: The Hybrid Elevated Radio Observatory for Neutrinos (HERON) Project
The Hybrid Elevated Radio Observatory for Neutrinos (HERON) Project Open
Measuring ultra-high energy neutrinos, with energies above $10^{16}$ eV, is the next frontier of the emerging multi-messenger era. Their detection requires building a large-scale detector with 10 times the instantaneous sensitivity of curr…
View article: Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy
Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy Open
Detecting ultrahigh-energy neutrinos can take two complementary approaches with different trade-offs. 1)~Wide and shallow: aim for the largest effective volume, and to be cost-effective, go for wide field-of-view but at the cost of a shall…
View article: The Low Frequency Instrument for the Payload for Ultrahigh Energy Observations (PUEO)
The Low Frequency Instrument for the Payload for Ultrahigh Energy Observations (PUEO) Open
The Payload for Ultrahigh Energy Observations (PUEO) long-duration balloon experiment is designed to observe ultra-high energy (UHE) neutrinos with energies above EeV. PUEO consists of a Main Instrument (MI) on a fixed gondola and a Low Fr…
View article: Design of the PUEO Payload
Design of the PUEO Payload Open
The primary science goals of the Payload for Ultrahigh Energy Observations (PUEO) are testing models of both candidate sources of ultrahigh-energy neutrinos (UHEN) and the propagation of ultrahigh-energy cosmic rays. PUEO is a balloon-born…
View article: Targeting 100-PeV tau neutrino detection with an array of phased and high-gain reconstruction antennas
Targeting 100-PeV tau neutrino detection with an array of phased and high-gain reconstruction antennas Open
Neutrinos at ultrahigh energies can originate both from interactions of cosmic rays at their acceleration sites and through cosmic-ray interactions as they propagate through the universe. These neutrinos are expected to have a low flux whi…
View article: Sensitivity of BEACON to Ultrahigh Energy Neutrinos
Sensitivity of BEACON to Ultrahigh Energy Neutrinos Open
The Beamforming Elevated Array for COsmic Neutrinos (BEACON) is a proposed detector concept consisting of many phased radio antenna arrays placed on mountaintops, searching for the upgoing extensive air showers created by Earth-skimming ta…
View article: Searching for Cosmic Rays with the BEACON Prototype
Searching for Cosmic Rays with the BEACON Prototype Open
A cosmic ray search with the prototype for the Beamforming Elevated Array for COsmic Neutrinos\n(BEACON) helps characterize the BEACON instrument, including the RF trigger that is ultimately\ncrucial for detecting tau-neutrino induced geom…
View article: Searching for Askaryan Emission from Neutrinos with the Payload for Ultrahigh Energy Observations (PUEO)
Searching for Askaryan Emission from Neutrinos with the Payload for Ultrahigh Energy Observations (PUEO) Open
The Payload for Ultrahigh Energy Observations (PUEO) is a long-duration balloon payload under construction scheduled to fly over Antarctica in late 2025. PUEO will deploy a broadband interferometric radio telescope pointing down at the ice…
View article: Design of the next-generation ultrahigh energy neutrino observatory PUEO
Design of the next-generation ultrahigh energy neutrino observatory PUEO Open
PUEO (the Payload for Ultrahigh Energy Observations) is a balloon-borne payload designed to detect the impulsive radio signals produced through the Askaryan effect by ultrahigh-energy (UHE) neutrinos (>1 EeV) in the Antarctic ice. Several …
View article: Identifying and Characterizing Air Shower Events with the Payload for Ultrahigh Energy Observations (PUEO)
Identifying and Characterizing Air Shower Events with the Payload for Ultrahigh Energy Observations (PUEO) Open
The Payload for Ultrahigh Energy Observations (PUEO) is a balloon-borne neutrino observatory currently under construction and slated to fly in December 2025. PUEO will be sensitive to both Askaryan radio emission from neutrino interactions…
View article: Detection of Radio Emission by Cosmic Rays with the BEACON Prototype
Detection of Radio Emission by Cosmic Rays with the BEACON Prototype Open
The Beamforming Elevated Array for COsmic Neutrinos (BEACON) is a novel detector concept\nconsisting of many radio interferometers placed on mountaintops, searching for the radio emission\nof upgoing extensive air showers created when ultr…
View article: Sensitivity of BEACON to Point Sources of Ultrahigh Energy Neutrinos
Sensitivity of BEACON to Point Sources of Ultrahigh Energy Neutrinos Open
The Beamforming Elevated Array for COsmic Neutrinos (BEACON) is a novel detector concept\ndesigned to measure the tau neutrino flux above 100 PeV. BEACON consists of multiple radio\ninterferometers placed on mountaintops which search for t…
View article: Updated Simulation of Airborne Neutrino Detectors for the PUEO Experiment
Updated Simulation of Airborne Neutrino Detectors for the PUEO Experiment Open
The upcoming Payload for Ultra-high Energy Observations (PUEO) experiment is planned for launch in the 2025/2026 season, and detailed simulation of the experiment is necessary for both the design of the instrument prior to launch, as well …
View article: The Beamforming Elevated Array for COsmic Neutrinos (BEACON): A Radio Detector for Earth-Skimming Tau Neutrinos
The Beamforming Elevated Array for COsmic Neutrinos (BEACON): A Radio Detector for Earth-Skimming Tau Neutrinos Open
When ultrahigh energy tau neutrinos skim the Earth, they can generate tau leptons that then decay in the atmosphere, forming upgoing extensive air showers. The Beamforming Elevated Array\nfor COsmic Neutrinos (BEACON) is a novel detector c…
View article: Analysis of a tau neutrino origin for the near-horizon air shower events observed by the fourth flight of the Antarctic Impulsive Transient Antenna
Analysis of a tau neutrino origin for the near-horizon air shower events observed by the fourth flight of the Antarctic Impulsive Transient Antenna Open
We study in detail the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to possible Formula Presented point source fluxes detected via Formula Presented-lepton-induced air showers. This investigation is framed around the ob…
View article: Analysis of a Tau Neutrino Origin for the Near-Horizon Air Shower Events Observed by the Fourth Flight of the Antarctic Impulsive Transient Antenna (ANITA)
Analysis of a Tau Neutrino Origin for the Near-Horizon Air Shower Events Observed by the Fourth Flight of the Antarctic Impulsive Transient Antenna (ANITA) Open
We study in detail the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to possible $ν_τ$ point source fluxes detected via $τ$-lepton-induced air showers. This investigation is framed around the observation of four upward-g…
View article: The Payload for Ultrahigh Energy Observations (PUEO): a white paper
The Payload for Ultrahigh Energy Observations (PUEO): a white paper Open
The Payload for Ultrahigh Energy Observations (PUEO) long-duration balloon\nexperiment is designed to have world-leading sensitivity to ultrahigh-energy\nneutrinos at energies above 1 EeV. Probing this energy region is essential for\nunder…
View article: Discovering the Highest Energy Neutrinos with the Payload for Ultrahigh Energy Observations (PUEO)
Discovering the Highest Energy Neutrinos with the Payload for Ultrahigh Energy Observations (PUEO) Open
The Payload for Ultrahigh Energy Observations (PUEO) is a NASA Long-Duration Balloon Mission that has been selected for concept development. PUEO has unprecedented sensitivity to ultra-high energy neutrinos above $10^{18}$ eV. PUEO will be…
View article: Modeling and Validating RF-Only Interferometric Triggering with Cosmic Rays for BEACON
Modeling and Validating RF-Only Interferometric Triggering with Cosmic Rays for BEACON Open
When Earth-skimming tau neutrinos interact within the Earth, they generate upgoing tau leptons that can decay in the atmosphere, forming extensive air showers. The Beamforming Elevated Array for COsmic Neutrinos (BEACON) is a novel detecto…
View article: Searching for RF-Only Triggered Cosmic Ray Events with the High-Elevation BEACON Prototype
Searching for RF-Only Triggered Cosmic Ray Events with the High-Elevation BEACON Prototype Open
The Beamforming Elevated Array for COsmic Neutrinos (BEACON) is a concept for a neutrino telescope designed to measure tau lepton air showers generated from tau neutrino interactions near the horizon. This detection mechanism provides a pu…
View article: Sensitivity of BEACON to Point Sources of Tau Neutrinos
Sensitivity of BEACON to Point Sources of Tau Neutrinos Open