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Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
A high-energy neutrino event detected by IceCube on 22 September 2017 was coincident in direction and time with a gamma-ray flare from the blazar TXS 0506+056. Prompted by this association, we inveExpand
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Radio Luminosity, Black Hole Mass and Eddington Ratio for Quasars from the Sloan Digital Sky Survey
We investigate the M-BH-sigma* relation for radio-loud quasars with redshift z < 0.83 in Data Release 3 of the Sloan Digital Sky Survey (SDSS). The sample consists of 3772 quasars with better modelsExpand
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Neutrino oscillation studies with IceCube-DeepCore
IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to search for astrophysical neutrinos with energies of PeV and higher. This goal has been achieved withExpand
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Cosmic ray spectrum and composition from PeV to EeV using 3 years of data from IceTop and IceCube
We report on measurements of the all-particle cosmic ray energy spectrum and composition in the PeV to EeV energy range using 3 years of data from the IceCube Neutrino Observatory. The IceTopExpand
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Ab Initio Calculation of structures and properties of halogenated general anesthetics: halothane and sevoflurane
To correctly analyze the effects of general anesthetics on their potential targets by large‐scale molecular simulation, the structural parameters and partial atomic charges of the anesthetics are ofExpand
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In the title compound, C18H13N5, the two pyridyl rings form dihedral angles of 32.7 (2) and 30.1 (2)° with the triazole ring. The most favoured orientation of the pyridyl rings is that with their NExpand
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Superconvergence of Local Discontinuous Galerkin Method for One-Dimensional Linear Schrödinger Equations
In this paper, we study the superconvergence properties of the LDG method for the one-dimensional linear Schrödinger equation. Expand
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The title compound, [Co(C6H4NO2)2]n, contains chiral two-dimensional layers assembled from Co2+ cations and nicotin­ate anions. Expand
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Explaining the rolling‐pin distribution of suprathermal electrons behind dipolarization fronts
The rolling-pin distribution of suprathermal electrons (40-200 keV), showing electron pitch angles primarily at 0°, 90°, and 180°, has recently been reported behind dipolarization fronts (DFs) bothExpand
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