activity
20072021
most citedMulti-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A

1.1k citations · 12k across the 112 of their papers we have counts for

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Showing astro-ph.HEShow all

83 papers · 1 filter

astro-ph.HE2021★ 19 cited

Analysis of a Tau Neutrino Origin for the Near-Horizon Air Shower Events Observed by the Fourth Flight of the Antarctic Impulsive Transient Antenna (ANITA)

R. Prechelt, S. A. Wissel, A. Romero-Wolf +65

We study in detail the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to possible point source fluxes detected via -lepton-induced air showers. This inve…

astro-ph.HE2020★ 6 cited

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★ 33 cited

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.HE2019★ 9 cited

The IceCube Neutrino Observatory -- Contributions to the 36th International Cosmic Ray Conference (ICRC2019)

IceCube Collaboration, M. G. Aartsen, M. Ackermann +355

Contributions from the IceCube Collaboration presented at the 36th International Cosmic Ray Conference, 24 July - 1 August 2019, Madison, Wisconsin, USA.

astro-ph.HE2019★ 102 cited

Constraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA

P. W. Gorham, P. Allison, O. Banerjee +57

The ANtarctic Impulsive Transient Antenna (ANITA) NASA long-duration balloon payload completed its fourth flight in December 2016, after 28 days of flight time. ANITA is sensitive…

astro-ph.HE2019★ 4 cited

Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +332

Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos with a typical energy cutoff well below 100 TeV. For the IceCube Neutrino Observa…