Observation of the top quark
…, P Ermolov, OV Eroshin, VN Evdokimov, S Fahey… - Physical review …, 1995 - APS
The D0 Collaboration reports on a search for the standard model top quark in pp collisions at
s= 1.8 TeV at the Fermilab Tevatron with an integrated luminosity of approximately 50 pb− 1…
s= 1.8 TeV at the Fermilab Tevatron with an integrated luminosity of approximately 50 pb− 1…
The DØ detector
…, O Eroshin, V Evdokimov, S Fahey… - Nuclear Instruments and …, 1994 - Elsevier
… The DO detector has been constructed to study proton-antiproton collisions at v~'s =2 TeV
in the Fermilab Tevatron collider. The experiment was first provisionally approved in 1983 and …
in the Fermilab Tevatron collider. The experiment was first provisionally approved in 1983 and …
Neutrino emission from the direction of the blazar TXS 0506+ 056 prior to the IceCube-170922A alert
… The height of each line indicates the event weight: the product of the event’s spatial term …
[A distribution for the true neutrino energy of a single event can also be inferred from the event’s …
[A distribution for the true neutrino energy of a single event can also be inferred from the event’s …
The IceCube Neutrino Observatory: instrumentation and online systems
…, P Eller, S Euler, PA Evenson, S Fahey… - Journal of …, 2017 - iopscience.iop.org
In the six decades following the discovery of the neutrino by Cowan and Reines [1], detectors
have been realized that have explored the properties and sources of neutrinos. Early …
have been realized that have explored the properties and sources of neutrinos. Early …
The role of chemokines in acute and chronic hepatitis C infection
S Fahey, E Dempsey, A Long - Cellular & Molecular Immunology, 2014 - nature.com
Hepatitis C imposes a significant burden on global healthcare. Chronic infection is associated
with progressive inflammation of the liver which typically manifests in cirrhosis, organ …
with progressive inflammation of the liver which typically manifests in cirrhosis, organ …
IceCube-Gen2: the window to the extreme Universe
…, JJ Evans, PA Evenson, S Fahey… - Journal of Physics G …, 2021 - iopscience.iop.org
The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided
a wealth of information about the Universe. However, at PeV (10 15 eV) energies and above, …
a wealth of information about the Universe. However, at PeV (10 15 eV) energies and above, …
Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A
…, T Ehrhardt, B Eichmann, P Eller, P Evenson, S Fahey… - Science, 2018 - science.org
INTRODUCTION Neutrinos are tracers of cosmic-ray acceleration: electrically neutral and
traveling at nearly the speed of light, they can escape the densest environments and may be …
traveling at nearly the speed of light, they can escape the densest environments and may be …
Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
…, P Eller, S Euler, PA Evenson, S Fahey… - The Astrophysical …, 2016 - iopscience.iop.org
The detection of high-energy cosmic neutrinos as cosmic messengers has been an
important goal of astroparticle physics. Being stable, electrically neutral particles, high-energy …
important goal of astroparticle physics. Being stable, electrically neutral particles, high-energy …
A combined maximum-likelihood analysis of the high-energy astrophysical neutrino flux measured with IceCube
…, S Euler, PA Evenson, O Fadiran, S Fahey… - The Astrophysical …, 2015 - iopscience.iop.org
… Fahey 6 , AR Fazely 35 , A. Fedynitch 17 , J. Feintzeig 6 , J. … Receive alerts on all new
research papers in American Astronomical Society (A A S ) journals as soon as they are …
research papers in American Astronomical Society (A A S ) journals as soon as they are …
IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data
…, PA Evenson, S Fahey, AR Fazely, S Fiedlschuster… - Physical Review D, 2021 - APS
The IceCube Neutrino Observatory has established the existence of a high-energy all-sky
neutrino flux of astrophysical origin. This discovery was made using events interacting within a …
neutrino flux of astrophysical origin. This discovery was made using events interacting within a …