• Corpus ID: 119206924

Pierre Auger Observatory and Telescope Array: Joint Contributions to the 35th International Cosmic Ray Conference (ICRC 2017)

  title={Pierre Auger Observatory and Telescope Array: Joint Contributions to the 35th International Cosmic Ray Conference (ICRC 2017)},
  author={the Event Horizon Telescope Collaboration and The Pierre Auger Collaboration},
Joint contributions of the Telescope Array Collaboration and the Pierre Auger Collaboration to the 35th International Cosmic Ray Conference (ICRC 2017), 12-20 July 2017, Bexco, Busan, Korea. 

The Giant Radio Array for Neutrino Detection (GRAND): Science and design

The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the

KLYPVE-EUSO: Science and UHECR observational capabilities

The study of Ultra High Energy Cosmic Rays (UHECRs) offers unique possibilities to probe the energies currently inaccessible by man-made accelerators. The last years have shed light on several

The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) observatory

The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to accurately observe ultra-high-energy cosmic rays (UHECRs) and cosmic neutrinos from space with sensitivity over the full

Searches for correlation between UHECR events and high-energy gamma-ray Fermi-LAT data

The astrophysical sources responsible for ultra high-energy cosmic rays (UHECRs) continue to be one of the most intriguing mysteries in astrophysics. We present a comprehensive search for

A Giant Radio Array for Neutrino Detection (GRAND)

  • S. D. Jong
  • Physics
    Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020)
  • 2021
This poster presents the results of a two-year research project aimed at determining the genetic basis of canine coronavirus, which has attacked the immune system in dogs and is believed to have killed at least three animals.

Measurement of the chemical composition of ultra high energy cosmic rays with the HEAT telescopes of the Pierre Auger Observatory

The Pierre Auger Observatory is currently the largest detector for measurements of cosmic rays with energies beyond 1018 eV. It uses a hybrid detection method with fluorescence telescopes and surface

First results from the TUS orbital detector in the extensive air shower mode

TUS (Tracking Ultraviolet Set-up), the first orbital detector of extreme energy cosmic rays (EECRs), those with energies above 50 EeV, was launched into orbit on April 28, 2016, as a part of the

Open Questions in Cosmic-Ray Research at Ultrahigh Energies

We review open questions and prospects for progress in ultrahigh-energy cosmicray (UHECR) research, based on a series of discussions that took place during the “The High-Energy Universe: Gamma-Ray,

Dissecting the region around IceCube-170922A: the blazar TXS 0506+056 as the first cosmic neutrino source

We present the dissection in space, time, and energy of the region around the IceCube-170922A neutrino alert. This study is motivated by: (1) the first association between a neutrino alert and a

What is the nature and origin of the highest-energy particles in the universe?

This white paper was submitted to the US Astronomy and Astrophysics Decadal Survey (Astro2020) and defines the science questions to be answered in the next decade in the field of Ultra-High Energy