activity
20172024
most citedConstraints and prospects on gravitational wave and neutrino emission using GW150914

5 citations · 6 across the 3 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2021

A Time-Variability Test for Candidate Neutrino Sources Observed with IceCube

Pranav Dave

Recent studies with IceCube have shown signs of a time-integrated flux of astrophysical neutrinos from point-like sources such as TXS 0506+056 and NGC 1068. Time-variability of thi…

hep-ex2020

Measurement of the high-energy all-flavor neutrino-nucleon cross section with IceCube

R. Abbasi, M. Ackermann, J. Adams +361

The flux of high-energy neutrinos passing through the Earth is attenuated due to their interactions with matter. The interaction rate is modulated by the neutrino interaction cross…

astro-ph.IM20201 cited

Deep-sea deployment of the KM3NeT neutrino telescope detection units by self-unrolling

The KM3NeT Collaboration, S. Aiello, A. Albert +252

KM3NeT is a research infrastructure being installed in the deep Mediterranean Sea. It will house a neutrino telescope comprising hundreds of networked moorings - detection units or…

astro-ph.HE2020

IceCube Search for High-Energy Neutrino Emission from TeV Pulsar Wind Nebulae

M. G. Aartsen, M. Ackermann, J. Adams +361

Pulsar wind nebulae (PWNe) are the main gamma-ray emitters in the Galactic plane. They are diffuse nebulae that emit nonthermal radiation. Pulsar winds, relativistic magnetized out…

astro-ph.HE2019

Search for dark matter towards the Galactic Centre with 11 years of ANTARES data

The ANTARES Collaboration

Neutrino detectors participate in the indirect search for the fundamental constituents of dark matter (DM) in form of weakly interacting massive particles (WIMPs). In WIMP scenario…

astro-ph.HE2019

Low Energy Cosmic Ray Spectrum from 250 TeV to 10 PeV using IceTop

Ramesh Koirala, Thomas K. Gaisser

Using IceTop, the surface component of the IceCube Neutrino Observatory, the all-particle cosmic ray energy spectrum has been determined above a few PeV. The measured energy spectr…