Proposes the Trinity air-shower imaging system for detecting ultrahigh energy tau neutrinos between 10^7 and 10^10 GeV to address IceCube neutrino sources, UHECR origins, and high-energy neutrino physics.
The Pierre Auger Observatory: Contributions to the 35th International Cosmic Ray Conference (ICRC 2017)
3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
abstract
Contributions of the Pierre Auger Collaboration to the 35th International Cosmic Ray Conference (ICRC 2017), 12-20 July 2017, Bexco, Busan, Korea.
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2019 3verdicts
UNVERDICTED 3representative citing papers
Assuming starbursts source UHECRs, arrival directions (especially a TA hot spot from M82) can constrain Galactic magnetic field models.
POEMMA is a proposed NASA probe-class mission designed to observe ultra-high energy cosmic rays and cosmic neutrinos from space.
citing papers explorer
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Trinity: An Air-Shower Imaging Instrument to detect Ultrahigh Energy Neutrinos
Proposes the Trinity air-shower imaging system for detecting ultrahigh energy tau neutrinos between 10^7 and 10^10 GeV to address IceCube neutrino sources, UHECR origins, and high-energy neutrino physics.
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The Galactic magnetic field in the light of starburst-generated ultrahigh-energy cosmic rays
Assuming starbursts source UHECRs, arrival directions (especially a TA hot spot from M82) can constrain Galactic magnetic field models.
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POEMMA (Probe of Extreme Multi-Messenger Astrophysics) design
POEMMA is a proposed NASA probe-class mission designed to observe ultra-high energy cosmic rays and cosmic neutrinos from space.