activity
20182022
most citedConstraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA

102 citations · 112 across the 3 of their papers we have counts for

collaborators

17 papers

astro-ph.HE202210 cited

Advancing the Landscape of Multimessenger Science in the Next Decade

Kristi Engel, Tiffany Lewis, Marco Stein Muzio +91

The last decade has brought about a profound transformation in multimessenger science. Ten years ago, facilities had been built or were under construction that would eventually dis…

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

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…