Christopher Persichilli
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View article: Modelling of the above-ground biomass and ecological composition of semi-natural grasslands on the strenght of remote sensing data and machine learning algorithms
Modelling of the above-ground biomass and ecological composition of semi-natural grasslands on the strenght of remote sensing data and machine learning algorithms Open
Semi-natural grasslands represent a vital source of forage and fodder for livestock farming, fulfilling an essential ecological function. This study upholded the efficacy of Sentinel-2 time series data in conjunction with ground data on ab…
View article: Developing new analysis tools for near surface radio-based neutrino detectors
Developing new analysis tools for near surface radio-based neutrino detectors Open
The ARIANNA experiment is an Askaryan radio detector designed to measure high-energy neutrino induced cascades within the Antarctic ice. Ultra-high-energy neutrinos above 10 16 eV have an extremely low flux, so experimental data captured a…
View article: TAROGE-M: Antarctic High-Mountain Radio Antenna Array for Detecting Ultra-High Energy ANITA Anomalous Events
TAROGE-M: Antarctic High-Mountain Radio Antenna Array for Detecting Ultra-High Energy ANITA Anomalous Events Open
TAROGE-M is a radio antenna array atop $\sim2.7$ km-high Mt.~Melbourne in Antarctica for detecting ultra-high energy (UHE, $E> 10^{17}$ eV) air showers in near-horizontal directions. Besides the detection of cosmic rays and Earth-skimming …
View article: Developing New Analysis Tools for Near Surface Radio-based Neutrino Detectors
Developing New Analysis Tools for Near Surface Radio-based Neutrino Detectors Open
The ARIANNA experiment is an Askaryan radio detector designed to measure high-energy neutrino induced cascades within the Antarctic ice. Ultra-high-energy neutrinos above $10^{16}$ eV have an extremely low flux, so experimental data captur…
View article: TAROGE-M: radio antenna array on antarctic high mountain for detecting near-horizontal ultra-high energy air showers
TAROGE-M: radio antenna array on antarctic high mountain for detecting near-horizontal ultra-high energy air showers Open
The TAROGE-M radio observatory is a self-triggered antenna array on top of the ∼2700 m high Mt. Melbourne in Antarctica, designed to detect impulsive geomagnetic emission from extensive air showers induced by ultra-high energy (UHE) partic…
View article: TAROGE-M: Radio Antenna Array on Antarctic High Mountain for Detecting Near-Horizontal Ultra-High Energy Air Showers
TAROGE-M: Radio Antenna Array on Antarctic High Mountain for Detecting Near-Horizontal Ultra-High Energy Air Showers Open
TAROGE-M is a self-triggered radio antenna array atop the 2700 m high Mt. Melbourne in Antarctica, designed to detect impulsive geomagnetic emission from extensive air showers induced by ultra-high energy (UHE) particles beyond 0.1 EeV, in…
View article: Capabilities of ARIANNA: Neutrino Pointing Resolution and Implications for Future Ultra-high Energy Neutrino Astronomy
Capabilities of ARIANNA: Neutrino Pointing Resolution and Implications for Future Ultra-high Energy Neutrino Astronomy Open
A radio-frequency polarization measurement by the ARIANNA surface station was performed using a residual hole from the South Pole Ice Core (SPICEcore) Project. Radio pulses were emitted from a transmitter located down to 1.7 km below the s…
View article: Polarization Reconstruction of Cosmic Rays with the ARIANNA Neutrino Radio Detector
Polarization Reconstruction of Cosmic Rays with the ARIANNA Neutrino Radio Detector Open
The ARIANNA detector is designed to detect neutrinos of energies above 10 PeV. Due to the similarities in generated radio signals, cosmic rays are often used as test beams for neutrino detectors. Some ARIANNA detector stations are equipped…
View article: Science case and detector concept for ARIANNA high energy neutrino telescope at Moore's Bay, Antarctica
Science case and detector concept for ARIANNA high energy neutrino telescope at Moore's Bay, Antarctica Open
The ARIANNA neutrino detector, located at sea-level on the Ross Ice Shelf, Antarctica, consists of 200 autonomous and independent detector stations separated by 1 kilometer in a uniform triangular mesh, and serves to inform the planning of…
View article: A novel trigger based on neural networks for radio neutrino detectors
A novel trigger based on neural networks for radio neutrino detectors Open
The ARIANNA experiment is a proposed Askaryan detector designed to record radio signals induced by neutrino interactions in the Antarctic ice. Because of the low neutrino flux at high energies, the physics output is limited by statistics. …
View article: TAROGE-M: Radio Observatory on Antarctic High Mountain for Detecting Near-Horizon Ultra-High Energy Air Showers
TAROGE-M: Radio Observatory on Antarctic High Mountain for Detecting Near-Horizon Ultra-High Energy Air Showers Open
The TAROGE-M observatory is an autonomous antenna array on the top of Mt.~Melbourne ($\sim2700$ m altitude) in Antarctica, designed to detect radio pulses from ultra-high energy (over $10^{17}$ eV) air showers coming from near-horizon dire…
View article: Development of an in-situ calibration device of firn properties for Askaryan neutrino detectors
Development of an in-situ calibration device of firn properties for Askaryan neutrino detectors Open
High energy neutrinos ($E>10^{17}$ eV) are detected cost-efficiently via the Askaryan effect in ice, where a particle cascade induced by the neutrino interaction produces coherent radio emission that can be picked up by antennas installed …
View article: Neutrino vertex reconstruction with in-ice radio detectors using surface reflections and implications for the neutrino energy resolution
Neutrino vertex reconstruction with in-ice radio detectors using surface reflections and implications for the neutrino energy resolution Open
Ultra high energy neutrinos (Eν > 1016.5eV) are efficiently measured via radio signals following a neutrino interaction in ice. An antenna placed1Script O(15 m) below the ice surface will measure two signals for the vast majority of events…
View article: Performance of the ARIANNA pilot array, and implications for the next generation of UHE neutrino detectors
Performance of the ARIANNA pilot array, and implications for the next generation of UHE neutrino detectors Open
The seven-station test-bed for the ARIANNA ultra-high energy (UHE) neutrino telescope, the Hexagonal Radio Array (HRA), was completed during the 2014-2015 Antarctic summer season. In the more than four years since, the ARIANNA pilot array …
View article: NuRadioMC - Simulation Code for the Next Generation of Radio Neutrino Detectors
NuRadioMC - Simulation Code for the Next Generation of Radio Neutrino Detectors Open
The detection of astrophysical neutrinos by IceCube has opened a new window for the obser- vation of our universe. The use of antennas for detecting astroparticles has been proven useful and accurate after many years of radio cosmic-ray de…
View article: NuRadioReco: A new reconstruction framework for radio neutrino detectors
NuRadioReco: A new reconstruction framework for radio neutrino detectors Open
The radio detection of high-energy neutrinos has huge potential as it allows for cost-efficient instrumentation of huge volumes leading to unprecedented sensitivity in the $10^{16}~\mathrm{eV}$ - $10^{20}~\mathrm{eV}$ energy regime. The re…
View article: Observation of classically `forbidden' electromagnetic wave propagation and implications for neutrino detection.
Observation of classically `forbidden' electromagnetic wave propagation and implications for neutrino detection. Open
Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neutrino with an ice molecule. An array of RF antennas, deploye…
View article: Performance and Simulation of the ARIANNA Pilot Array, with Implications for Future Ultra-high Energy Neutrino Astronomy
Performance and Simulation of the ARIANNA Pilot Array, with Implications for Future Ultra-high Energy Neutrino Astronomy Open
The ARIANNA pilot Hexagonal Radio Array (HRA), a seven station test-bed for the development of an ultra-high energy (UHE) neutrino telescope, using Antarctica's Ross Ice Shelf as a detector, was completed during the 2014-2015 Antarctic sum…
View article: Radio search for EHE neutrinos with the ARIANNA pilot array, and ARIANNA performance projections
Radio search for EHE neutrinos with the ARIANNA pilot array, and ARIANNA performance projections Open
The ARIANNA project seeks to observe cosmogenic neutrinos with energy in excess of $10^{16}{eV}$ through the use of a grid of over 1000 independent radio detector stations. These stations search for the characteristic Askaryan radio pulses…
View article: Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf
Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf Open
The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. Here this articl…