activity
19982024
most citedAntennas for the Detection of Radio Emission Pulses from Cosmic-Ray induced Air Showers at the Pierre Auger Observatory

148 citations · 786 across the 43 of their papers we have counts for

collaborators
Showing 2019Show all

14 papers · 1 filter

astro-ph.HE2019

Contributions to the 36th International Cosmic Ray Conference (ICRC 2019) of the JEM-EUSO Collaboration

G. Abdellaoui, S. Abe, J. H. Adams +309

Compilation of papers presented by the JEM-EUSO Collaboration at the 36th International Cosmic Ray Conference (ICRC), held July 24 through August 1, 2019 in Madison, Wisconsin.

astro-ph.HE2019

The Pierre Auger Observatory: Contributions to the 36th International Cosmic Ray Conference (ICRC 2019)

The Pierre Auger Collaboration, A. Aab, P. Abreu +383

Contributions of the Pierre Auger Collaboration to the 36th International Cosmic Ray Conference (ICRC 2019), 24 July - 1 August 2019, Madison, Wisconsin, USA.

astro-ph.IM2019

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

A. V. Olinto, J. H. Adams, R. Aloisio +42

The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to observe cosmic neutrinos (CNs) above 20 PeV and ultra-high energy cosmic rays (UHECRs) above 20 EeV over t…

astro-ph.HE2019

Estimation of the exposure for the air shower detection mode of EUSO-SPB1

K. Shinozaki, M. Bertaina, F. Bisconti +11

EUSO-SPB1 was a balloon-borne pathfinder mission of the JEM-EUSO (Joint Experiment Missions for the Extreme Universe Space Observatory) program. A 12-day long flight started from N…

astro-ph.IM2019

UCIRC2: An Infrared Cloud Monitor for EUSO-SPB2

Rebecca Diesing, Khadijat Durojaiye, Seamus Flannery +6

We describe the design and implementation of the University of Chicago Infrared Camera 2 (UCIRC2) built for monitoring cloud coverage during the EUSO-SPB2 flight (the second genera…

astro-ph.HE2019

A new calculation of Earth-skimming very- and ultra-high energy tau neutrinos

Mary Hall Reno, Tonia M. Venters, John F. Krizmanic +3

Cosmic neutrinos above a PeV are produced either within astrophysical sources or when ultra-high energy cosmic rays interact in transit through the cosmic background radiation. Det…