activity
20132021
most citedConstraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA

102 citations · 156 across the 4 of their papers we have counts for

collaborators

25 papers

astro-ph.HE2021

The IceCube-Gen2 Collaboration -- Contributions to the 37th International Cosmic Ray Conference (ICRC2021)

Gen2 Collaboration, R. Abbasi, M. Ackermann +437

IceCube-Gen2 is a planned extension of the IceCube Neutrino Observatory at the South Pole. The extension is optimized to search for sources of astrophysical neutrinos from TeV to E…

astro-ph.IM2020

The Payload for Ultrahigh Energy Observations (PUEO): A White Paper

Q. Abarr, P. Allison, J. Ammerman Yebra +47

The Payload for Ultrahigh Energy Observations (PUEO) long-duration balloon experiment is designed to have world-leading sensitivity to ultrahigh-energy neutrinos at energies above…

astro-ph.HE2020

A search for ultrahigh-energy neutrinos associated with astrophysical sources using the third flight of ANITA

C. Deaconu, L. Batten, P. Allison +60

The ANtarctic Impulsive Transient Antenna (ANITA) long-duration balloon experiment is sensitive to interactions of ultra high-energy (E > 10^{18} eV) neutrinos in the Antarctic ice…

astro-ph.HE2020

Revisiting AGN as the Source of IceCube's Diffuse Neutrino Flux

Daniel Smith, Dan Hooper, Abigail Vieregg

The origin of the astrophysical neutrino flux reported by the IceCube Collaboration remains an open question. In this study, we use three years of publicly available IceCube data t…

astro-ph.HE2020

Unusual Near-horizon Cosmic-ray-like Events Observed by ANITA-IV

ANITA Collaboration, P. W. Gorham, A. Ludwig +57

ANITA's fourth long-duration balloon flight in late 2016 detected 29 cosmic-ray (CR)-like events on a background of anthropogenic events. CRs are mainly seen…

astro-ph.IM2020

Prospects for High-Elevation Radio Detection of >100 PeV Tau Neutrinos

Stephanie Wissel, Andrés Romero-Wolf, Harm Schoorlemmer +16

Tau neutrinos are expected to comprise roughly one third of both the astrophysical and cosmogenic neutrino flux, but currently the flavor ratio is poorly constrained and the expect…