activity
20182025
most citedMulti-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A

1.1k citations · 5.9k across the 156 of their papers we have counts for

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Showing 2021Show all

18 papers · 1 filter

astro-ph.HE2021★ 53 cited

Search for GeV-scale Dark Matter Annihilation in the Sun with IceCube DeepCore

R. Abbasi, M. Ackermann, J. Adams +376

The Sun provides an excellent target for studying spin-dependent dark matter-proton scattering due to its high matter density and abundant hydrogen content. Dark matter particles f…

hep-ex2021★ 41 cited

Search for Quantum Gravity Using Astrophysical Neutrino Flavour with IceCube

R. Abbasi, M. Ackermann, J. Adams +378

Along their long propagation from production to detection, neutrino states undergo quantum interference which converts their types, or flavours. High-energy astrophysical neutrinos…

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…

physics.ins-det2021

Homogeneity of the Photocathode in the Hamamatsu R15458-02 Photomultiplier Tube

M. A. Unland Elorrieta, R. S. Busse, L. Classen +1

It is common practice to test the optical properties of photomultiplier tubes (PMTs) by illuminating the entire photocathode region from the front at once and measuring the average…

astro-ph.HE2021★ 30 cited

Search for Relativistic Magnetic Monopoles with Eight Years of IceCube Data

IceCube Collaboration, R. Abbasi, M. Ackermann +380

We present an all-sky 90\% confidence level upper limit on the cosmic flux of relativistic magnetic monopoles using 2886 days of IceCube data. The analysis was optimized for monopo…

astro-ph.HE2021

Measuring the Neutrino Cross Section Using 8 years of Upgoing Muon Neutrinos Observed with IceCube

S. Robertson

The IceCube Neutrino Observatory detects neutrinos at energies orders of magnitude higher than those available to current accelerators. Above 40 TeV, neutrinos traveling through th…