1.6k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- E. Hicks2 profiles18 · h 37
- R. Davies4 profiles14 · h 55
- D. Rosario3 profiles11 · h 54
- R. Riffel3 profiles11 · h 32
- T. Rector10 · h 15
- J. Pantaleone9 · h 20
- L. Burtscher8 · h 29
- T. Storchi-Bergmann8 · h 59
- C. R. Almeida2 profiles6 · h 36
- C. Ricci2 profiles6 · h 46
- D. Lutz2 profiles6 · h 88
- M. Pereira-Santaella6 · h 32
- University of Maryland, College ParkUS248 papers
- University of OxfordGB246 papers
- RWTH Aachen UniversityDE240 papers
- Chiba UniversityJP239 papers
- Université Libre de BruxellesBE239 papers
- Humboldt-Universität zu BerlinDE238 papers
- Lawrence Berkeley National LaboratoryUS237 papers
- University of CanterburyNZ237 papers
- Vrije Universiteit BrusselBE237 papers
- University of California, BerkeleyUS235 papers
- Georgia Institute of TechnologyUS233 papers
- Clark Atlanta UniversityUS230 papers
10 papers · 1 filter
Seismicity on Tidally Active Solid-Surface Worlds
T. A. Hurford, W. G. Henning, R. Maguire +8
Tidal interactions between planets or stars and the bodies that orbit them dissipate energy in their interiors. The energy dissipated drives internal heating and a fraction of that…
Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +325
The IceCube Collaboration has observed a high-energy astrophysical neutrino flux and recently found evidence for neutrino emission from the blazar TXS 0506+056. These results open…
Detection of the Temporal Variation of the Sun's Cosmic Ray Shadow with the IceCube Detector
IceCube Collaboration, M. G. Aartsen, M. Ackermann +326
We report on the observation of a deficit in the cosmic ray flux from the directions of the Moon and Sun with five years of data taken by the IceCube Neutrino Observatory. Between…
Measurements using the inelasticity distribution of multi-TeV neutrino interactions in IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +330
Inelasticity--the fraction of a neutrino's energy transferred to hadrons--is a quantity of interest in the study of astrophysical and atmospheric neutrino interactions at multi-TeV…
Joint constraints on Galactic diffuse neutrino emission from ANTARES and IceCube
A. Albert, M. André, M. Anghinolfi +454
The existence of diffuse Galactic neutrino production is expected from cosmic ray interactions with Galactic gas and radiation fields. Thus, neutrinos are a unique messenger offeri…
Constraints on Minute-Scale Transient Astrophysical Neutrino Sources
M. G. Aartsen, M. Ackermann, J. Adams +331
High-energy neutrino emission has been predicted for several short-lived astrophysical transients including gamma-ray bursts (GRBs), core-collapse supernovae with choked jets and n…
Differential limit on the extremely-high-energy cosmic neutrino flux in the presence of astrophysical background from nine years of IceCube data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +330
We report a quasi-differential upper limit on the extremely-high-energy (EHE) neutrino flux above GeV based on an analysis of nine years of IceCube data. The astro…
Resolving the nuclear obscuring disk in the Compton-thick Seyfert galaxy NGC5643 with ALMA
A. Alonso-Herrero, M. Pereira-Santaella, S. García-Burillo +19
We present ALMA Band 6 CO(2--1) line and rest-frame 232GHz continuum observations of the nearby Compton-thick Seyfert galaxy NGC5643 with angular resolutions 0.11-0.26arcsec…
Search for neutrinos from decaying dark matter with IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +327
With the observation of high-energy astrophysical neutrinos by the IceCube Neutrino Observatory, interest has risen in models of PeV-mass decaying dark matter particles to explain…
The SINS/zC-SINF survey of z~2 galaxy kinematics: SINFONI adaptive optics-assisted data and kiloparsec-scale emission line properties
N. M. Förster Schreiber, A. Renzini, C. Mancini +29
We present the "SINS/zC-SINF AO survey" of 35 star-forming galaxies, the largest sample with deep adaptive optics-assisted (AO) near-infrared integral field spectroscopy at z~2. Th…