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Limits on GeV-scale WIMP Annihilation in Dwarf Spheroidals with IceCube DeepCore Open

Abbasi, R., Ackermann, M., Adams, J, Agarwalla, S. K., Aguilar, J. A. , et al. · 2025

Dark matter is approximately five times more abundant than baryonic matter in the universe, but its physical nature continues to elude physicists. One potential candidate for dark matter is a weakly-interacting massive particle (WIMP), whi…

Limits on GeV-scale WIMP Annihilation in Dwarf Spheroidals with IceCube DeepCore Open

Abbasi, R., Ackermann, M., Adams, J, Agarwalla, S. K., Aguilar, J. A. , et al. · 2025

Dark matter is approximately five times more abundant than baryonic matter in the universe, but its physical nature continues to elude physicists. One potential candidate for dark matter is a weakly-interacting massive particle (WIMP), whi…

Search for GeV-scale Dark Matter from the Galactic Center with IceCube-DeepCore Open

The IceCube Collaboration, Abbasi, R., Ackermann, M, Adams, J., Agarwalla, S. K. , et al. · 2025

Models describing dark matter as a novel particle often predict that its annihilation or decay into Standard Model particles could produce a detectable neutrino flux in regions of high dark matter density, such as the Galactic Center. In t…

Search for GeV-scale Dark Matter from the Galactic Center with IceCube-DeepCore Open

the IceCube Collaboration, Abbasi, R., Ackermann, M., Adams, J., Agarwalla, S. K. , et al. · 2025

Models describing dark matter as a novel particle often predict that its annihilation or decay into Standard Model particles could produce a detectable neutrino flux in regions of high dark matter density, such as the Galactic Center. In t…

Measurement of the inelasticity distribution of neutrino-nucleon interactions for 80 GeV < E$_ν$ < 560 GeV with IceCube DeepCore Open

IceCube Collaboration, Abbasi, R., Ackermann, M., Adams, J, Agarwalla, S. K. , et al. · 2025

We report a study of the inelasticity distribution in the scattering of neutrinos of energy 80–560 GeV off nucleons. Using atmospheric muon neutrinos detected in IceCube’s sub-array DeepCore during 2012– 2021, we fit the observed inelastic…

Search for Relativistic Magnetic Monopoles with Eight Years of IceCube Data Open

Abbasi, R., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M. , et al. · 2022

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 monopole speeds between 0.750c and 0.995c, without any explicit re…

Velocity independent constraints on spin-dependent DM-nucleon interactions from IceCube and PICO Open

Aartsen, M. G., Ackermann, Markus, Adams, J., Aguilar, J. A., Ahlers, M. , et al. · 2020

Constraints on neutrino emission from nearby galaxies using the 2MASS redshift survey and IceCube Open

Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M. , et al. · 2020

The distribution of galaxies within the local universe is characterized by anisotropic features. Observatories searching for the production sites of astrophysical neutrinos can take advantage of these features to establish directional corr…

A Search for Neutrino Point-source Populations in 7 yr of IceCube Data with Neutrino-count Statistics Open

Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M. , et al. · 2020

The presence of a population of point sources in a data set modifies the underlying neutrino-count statistics from the Poisson distribution. This deviation can be exactly quantified using the non-Poissonian template fitting technique, and …

Search for PeV Gamma-Ray Emission from the Southern Hemisphere with 5 Yr of Data from the IceCube Observatory Open

Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M. , et al. · 2020

The measurement of diffuse PeV gamma-ray emission from the Galactic plane would provide information about the energy spectrum and propagation of Galactic cosmic rays, and the detection of a pointlike source of PeV gamma-rays would be stron…

Design and performance of the first IceAct demonstrator at the South Pole Open

Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M. , et al. · 2020

In this paper we describe the first results of a compact imaging air-Cherenkov telescope, IceAct, operating in coincidence with the IceCube Neutrino Observatory (IceCube) at the geographic South Pole. An array of IceAct telescopes (referre…

A Search for MeV to TeV Neutrinos from Fast Radio Bursts with IceCube Open

Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M. , et al. · 2020

We present two searches for IceCube neutrino events coincident with 28 fast radio bursts (FRBs) and 1 repeating FRB. The first improves on a previous IceCube analysis—searching for spatial and temporal correlation of events with FRBs at en…

Investigation of Two Fermi-LAT Gamma-Ray Blazars Coincident with High-energy Neutrinos Detected by IceCube Open

Garrappa, S., Buson, S., Franckowiak, A., Shappee, B. J., Beacom, J. F. , et al. · 2019

After the identification of the gamma-ray blazar TXS 0506+056 as the first compelling IceCube neutrino source candidate, we perform a systematic analysis of all high-energy neutrino events satisfying the IceCube realtime trigger criteria. …

Search for transient optical counterparts to high-energy IceCube neutrinos with Pan-STARRS1 Open

Kankare, E., Huber, M., Smartt, S. J., Chambers, K., Smith, K. W. , et al. · 2019

In order to identify the sources of the observed diffuse high-energy neutrino flux, it is crucial to discover their electromagnetic counterparts. To increase the sensitivity of detecting counterparts of transient or variable sources by tel…

Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data Open

Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M. , et al. · 2019

Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A Open

Aartsen, M. G., Ackermann, M., Adams, J, Aguilar, J. A., Ahlers, M. , et al. · 2018

Neutrino emission from a flaring blazar Neutrinos interact only very weakly with matter, but giant detectors have succeeded in detecting small numbers of astrophysical neutrinos. Aside from a diffuse background, only two individual sources…

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