S Westerhoff
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Explore the profile of S Westerhoff including associated specialties, affiliations and a list of published articles.
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Articles
28
Citations
75
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Recent Articles
1.
Aartsen M, Ackermann M, Adams J, Aguilar J, Ahlers M, Ahrens M, et al.
Eur Phys J C Part Fields
. 2020 Jan;
77(10):692.
PMID: 31997925
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 in...
2.
Aartsen M, Ackermann M, Adams J, Aguilar J, Ahlers M, Ahrens M, et al.
Eur Phys J C Part Fields
. 2019 Apr;
78(10):831.
PMID: 30930683
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 observed flux. We present...
3.
Aartsen M, Ackermann M, Adams J, Aguilar J, Ahlers M, Ahrens M, et al.
Phys Rev Lett
. 2019 Mar;
122(5):051102.
PMID: 30822017
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 neutron star mergers. IceCube's optical and x-ray follow-up program...
4.
Abeysekara A, Albert A, Alfaro R, Alvarez C, Alvarez J, Arceo R, et al.
Nature
. 2018 Nov;
564(7736):E38.
PMID: 30482938
In this Letter, owing to a production error, the penultimate version of the PDF was published. The HTML version was always correct. The PDF has been corrected online.
5.
Abeysekara A, Albert A, Alfaro R, Alvarez C, Alvarez J, Arceo R, et al.
Nature
. 2018 Oct;
562(7725):82-85.
PMID: 30283106
SS 433 is a binary system containing a supergiant star that is overflowing its Roche lobe with matter accreting onto a compact object (either a black hole or neutron star)....
6.
Aartsen M, Ackermann M, Adams J, Aguilar J, Ahlers M, Ahrens M, et al.
Phys Rev Lett
. 2018 Mar;
120(7):071801.
PMID: 29542976
We present a measurement of the atmospheric neutrino oscillation parameters using three years of data from the IceCube Neutrino Observatory. The DeepCore infill array in the center of IceCube enables...
7.
Abeysekara A, Albert A, Alfaro R, Alvarez C, Alvarez J, Arceo R, et al.
Science
. 2017 Nov;
358(6365):911-914.
PMID: 29146808
The unexpectedly high flux of cosmic-ray positrons detected at Earth may originate from nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary production. We report the detection, using...
8.
Aartsen M, Abraham K, Ackermann M, Adams J, Aguilar J, Ahlers M, et al.
Phys Rev Lett
. 2016 Dec;
117(24):241101.
PMID: 28009216
We report constraints on the sources of ultrahigh-energy cosmic rays (UHECRs) above 10^{9} GeV, based on an analysis of seven years of IceCube data. This analysis efficiently selects very high-...
9.
Aartsen M, Abraham K, Ackermann M, Adams J, Aguilar J, Ahlers M, et al.
Phys Rev Lett
. 2016 Aug;
117(7):071801.
PMID: 27563950
The IceCube neutrino telescope at the South Pole has measured the atmospheric muon neutrino spectrum as a function of zenith angle and energy in the approximate 320 GeV to 20 ...
10.
Aartsen M, Abraham K, Ackermann M, Adams J, Aguilar J, Ahlers M, et al.
Phys Rev Lett
. 2015 Sep;
115(8):081102.
PMID: 26340177
Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the existence of a high energy astrophysical neutrino flux utilizing a dominantly Southern Hemisphere data set consisting primarily...