activity
20022021
most citedExperimental and Theoretical Challenges in the Search for the Quark Gluon Plasma: The STAR Collaboration's Critical Assessment of the Evidence from RHIC Collisions

3.4k citations · 10.6k across the 55 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

12 papers · 1 filter

astro-ph.HE2021★ 241 cited

Improved Characterization of the Astrophysical Muon-Neutrino Flux with 9.5 Years of IceCube Data

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

We present a measurement of the high-energy astrophysical muon-neutrino flux with the IceCube Neutrino Observatory. The measurement uses a high-purity selection of ~650k neutrino-i…

astro-ph.HE2021★ 46 cited

A search for neutrino emission from cores of Active Galactic Nuclei

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

The sources of the majority of the high-energy astrophysical neutrinos observed with the IceCube neutrino telescope at the South Pole are unknown. So far, only a gamma-ray blazar w…

astro-ph.HE2021★ 15 cited

Search for GeV Neutrino Emission During Intense Gamma-Ray Solar Flares with the IceCube Neutrino Observatory

R. Abbasi, M. Ackermann, J. Adams +364

Solar flares convert magnetic energy into thermal and non-thermal plasma energy, the latter implying particle acceleration of charged particles such as protons. Protons are injecte…

astro-ph.HE2020★ 20 cited

A search for time-dependent astrophysical neutrino emission with IceCube data from 2012 to 2017

IceCube Collaboration, R. Abbasi, M. Ackermann +361

High-energy neutrinos are unique messengers of the high-energy universe, tracing the processes of cosmic-ray acceleration. This paper presents analyses focusing on time-dependent n…

astro-ph.HE2020★ 19 cited

Measurements of the Time-Dependent Cosmic-Ray Sun Shadow with Seven Years of IceCube Data -- Comparison with the Solar Cycle and Magnetic Field Models

M. G. Aartsen, R. Abbasi, M. Ackermann +376

Observations of the time-dependent cosmic-ray Sun shadow have been proven as a valuable diagnostic for the assessment of solar magnetic field models. In this paper, seven years of…

astro-ph.HE2020★ 38 cited

Cosmic Ray Spectrum from 250 TeV to 10 PeV using IceTop

IceCube Collaboration

We report here an extension of the measurement of the all-particle cosmic-ray spectrum with IceTop to lower energy. The new measurement gives full coverage of the knee region of th…

astro-ph.HE2019★ 450 cited

Time-integrated Neutrino Source Searches with 10 years of IceCube Data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +357

This paper presents the results from point-like neutrino source searches using ten years of IceCube data collected between Apr.~6, 2008 and Jul.~10, 2018. We evaluate the significa…

astro-ph.HE2019★ 165 cited

Cosmic Ray Spectrum and Composition from PeV to EeV Using 3 Years of Data From IceTop and IceCube

IceCube Collaboration

We report on measurements of the all-particle cosmic ray energy spectrum and composition in the PeV to EeV energy range using three years of data from the IceCube Neutrino Observat…

astro-ph.HE2017★ 15 cited

Measurement of the energy spectrum with IceCube-79

M. G. Aartsen, M. Ackermann, J. Adams +306

IceCube is a neutrino observatory deployed in the glacial ice at the geographic South Pole. The energy unfolding described in this paper is based on data taken with IceCube i…

astro-ph.HE2013★ 14 cited

The IceCube Neutrino Observatory Part IV: Searches for Dark Matter and Exotic Particles

IceCube Collaboration, M. G. Aartsen, R. Abbasi +278

Papers on searches for Dark Matter and exotic particles submitted to the 33nd International Cosmic Ray Conference (Rio de Janeiro 2013) by the IceCube Collaboration.

astro-ph.HE2010★ 154 cited

Measurement of the Anisotropy of Cosmic Ray Arrival Directions with IceCube

The IceCube Collaboration, R. Abbasi

We report the first observation of an anisotropy in the arrival direction of cosmic rays with energies in the multi TeV region in the Southern sky using data from the IceCube detec…

astro-ph.HE2010★ 76 cited

The Energy Spectrum of Atmospheric Neutrinos between 2 and 200 TeV with the AMANDA-II Detector

IceCube Collaboration, R. Abbasi

The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrin…