The Pacific Ocean Neutrino Experiment
arXiv:2005.09493 · doi:10.1038/s41550-020-1182-4
Abstract
The Pacific Ocean Neutrino Experiment (P-ONE) is a new initiative with a vision towards constructing a multi-cubic kilometre neutrino telescope, to expand our observable window of the Universe to highest energies, installed within the deep Pacific Ocean underwater infrastructure of Ocean Networks Canada.
arXiv comment17 pages, 2 Figures, submitted to Nature Astronomy
References in corpus (37)
- Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
- Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data
- Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
- The IceCube Neutrino Observatory: Instrumentation and Online Systems
- First observation of PeV-energy neutrinos with IceCube
- Active Galactic Nuclei: what's in a name?
- Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
- Time-integrated Neutrino Source Searches with 10 years of IceCube Data
- The IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data
- 3FHL: The Third Catalog of Hard Fermi-LAT Sources
- Characteristics of the diffuse astrophysical electron and tau neutrino flux with six years of IceCube high energy cascade data
- Differential limit on the extremely-high-energy cosmic neutrino flux in the presence of astrophysical background from nine years of IceCube data
- The Pacific Ocean Neutrino Experiment
- Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption
- Dissecting the region around IceCube-170922A: the blazar TXS 0506+056 as the first cosmic neutrino source
- The redshift of the BL Lac object TXS 0506+056
- Neutrino Fluxes from Active Galaxies: a Model-Independent Analysis
- Extreme blazars as counterparts of IceCube astrophysical neutrinos
- On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity
- Are both BL Lacs and pulsar wind nebulae the astrophysical counterparts of IceCube neutrino events?
- Transmission of light in deep sea water at the site of the Antares neutrino telescope
- First results of the Instrumentation Line for the deep-sea ANTARES neutrino telescope
- Extracting the Energy-Dependent Neutrino-Nucleon Cross Section Above 10 TeV Using IceCube Showers
- A simplified view of blazars: the neutrino background
- The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part II: Properties of the Atmospheric and Astrophysical Neutrino Flux
- Vetoing atmospheric neutrinos in a high energy neutrino telescope
- Dissecting the regions around IceCube high-energy neutrinos: growing evidence for the blazar connection
- Progress in unveiling extreme particle acceleration in persistent astrophysical jets
- Deep seawater inherent optical properties in the Southern Ionian Sea
- Connecting blazars with ultra high energy cosmic rays and astrophysical neutrinos
- New constraints on Heavy Neutral Leptons from Super-Kamiokande data
- Extragalactic gamma-ray background from AGN winds and star-forming galaxies in cosmological galaxy formation models
- Two-Year Optical Site Characterization for the Pacific Ocean Neutrino Experiment P-ONE in the Cascadia Basin
- Bracketing the impact of astrophysical uncertainties on local dark matter searches
- STRAW (STRings for Absorption length in Water): pathfinder for a neutrino telescope in the deep Pacific Ocean
- AGN outflows as neutrino sources: an observational test
- Bioluminescence modeling for deep sea experiments
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- SNR G54.1+0.3, a PeVatron candidate unveiled by LHAASO
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- Imprints of flavor anomalies on neutrino oscillations through dark matter halo
- Using Cosmic Rays to Predict the Weather: Meteorological Data Assimilation of Atmospheric Muon Flux Data
- Particle Astrophysics with High and Ultrahigh Energy Neutrinos