820 citations · 3.2k across the 24 of their papers we have counts for
24 papers
Large amplitude bidirectional anisotropy of cosmic-ray intensity observed with world-wide networks of ground-based neutron monitors and muon detectors in November, 2021
K. Munakata, M. Kozai, C. Kato +24
We analyze the cosmic-ray variations during a significant Forbush decrease observed with world-wide networks of ground-based neutron monitors and muon detectors during November 3-5…
Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube
A. Albert, M. Andre, M. Anghinolfi +1410
The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up…
Searches for Sterile Neutrinos with the IceCube Detector
The IceCube Collaboration
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 TeV r…
Multimessenger Search for Sources of Gravitational Waves and High-Energy Neutrinos: Results for Initial LIGO-Virgo and IceCube
The IceCube Collaboration, The LIGO Scientific Collaboration, The Virgo Collaboration +1185
We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neu…
Probing the origin of cosmic-rays with extremely high energy neutrinos using the IceCube Observatory
IceCube Collaboration, M. G. Aartsen, R. Abbasi +275
We have searched for extremely high energy neutrinos using data taken with the IceCube detector between May 2010 and May 2012. Two neutrino induced particle shower events with ener…
Energy Reconstruction Methods in the IceCube Neutrino Telescope
IceCube Collaboration, M. G. Aartsen, R. Abbasi +285
Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volume neutrino telescopes. The fundamental observable in such detectors is the Cher…
The IceCube Neutrino Observatory Part II: Atmospheric and Diffuse UHE Neutrino Searches of All Flavors
IceCube Collaboration, M. G. Aartsen, R. Abbasi +278
Papers on atmospheric and diffuse UHE neutrino searches of all flavors submitted to the 33nd International Cosmic Ray Conference (Rio de Janeiro 2013) by the IceCube Collaboration.
Measurement of Atmospheric Neutrino Oscillations with IceCube
The IceCube Collaboration
We present the first statistically significant detection of neutrino oscillations in the high-energy regime ( 20 GeV) from an analysis of IceCube Neutrino Observatory data colle…
First observation of PeV-energy neutrinos with IceCube
IceCube Collaboration, M. G. Aartsen, R. Abbasi +281
We report on the observation of two neutrino-induced events which have an estimated deposited energy in the IceCube detector of 1.04 0.16 and 1.14 0.17 PeV, respectivel…
Searching for soft relativistic jets in Core-collapse Supernovae with the IceCube Optical Follow-up Program
The IceCube Collaboration, R. Abbasi, Y. Abdou +262
Context. Transient neutrino sources such as Gamma-Ray Bursts (GRBs) and Supernovae (SNe) are hypothesized to emit bursts of high-energy neutrinos on a time-scale of \lesssim 100 s.…
The IceCube Neutrino Observatory II: All Sky Searches: Atmospheric, Diffuse and EHE
The IceCube Collaboration
All sky neutrino searches: Atmospheric neutrinos; Astrophysical neutrinos; Cosmegenic neutrinos; Submitted papers to the 32nd International Cosmic Ray Conference, Beijing 2011.
The Design and Performance of IceCube DeepCore
The IceCube Collaboration
The IceCube neutrino observatory in operation at the South Pole, Antarctica, comprises three distinct components: a large buried array for ultrahigh energy neutrino detection, a su…
Time-Integrated Searches for Point-like Sources of Neutrinos with the 40-String IceCube Detector
The IceCube Collaboration, R. Abbasi
We present the results of time-integrated searches for astrophysical neutrino sources in both the northern and southern skies. Data were collected using the partially-completed Ice…
Measurement of Acoustic Attenuation in South Pole Ice
the IceCube Collaboration
Using the South Pole Acoustic Test Setup (SPATS) and a retrievable transmitter deployed in holes drilled for the IceCube experiment, we have measured the attenuation of acoustic si…
Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector
The IceCube collaboration, R. Abbasi
A search for muon neutrinos from Kaluza-Klein dark matter annihilations in the Sun has been performed with the 22-string configuration of the IceCube neutrino detector using data c…
First Neutrino Point-Source Results From the 22-String IceCube Detector
IceCube Collaboration, R. Abbasi
We present new results of searches for neutrino point sources in the northern sky, using data recorded in 2007-08 with 22 strings of the IceCube detector (approximately one-fourth…
Limits on a muon flux from neutralino annihilations in the Sun with the IceCube 22-string detector
IceCube collaboration, R. Abbasi
A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live-time…
Solar Energetic Particle Spectrum on 13 December 2006 Determined by IceTop
R. Abbasi
On 13 December 2006 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop tanks, which are thick…
The IceCube Data Acquisition System: Signal Capture, Digitization, and Timestamping
The IceCube Collaboration
IceCube is a km-scale neutrino observatory under construction at the South Pole with sensors both in the deep ice (InIce) and on the surface (IceTop). The sensors, called Digital O…
Search for Point Sources of High Energy Neutrinos with Final Data from AMANDA-II
The IceCube Collaboration
We present a search for point sources of high energy neutrinos using 3.8 years of data recorded by AMANDA-II during 2000-2006. After reconstructing muon tracks and applying selecti…
Search for Ultra High-Energy Neutrinos with AMANDA-II
The IceCube Collaboration, M. Ackermann
A search for diffuse neutrinos with energies in excess of 10^5 GeV is conducted with AMANDA-II data recorded between 2000 and 2002. Above 10^7 GeV, the Earth is essentially opaque…
Exploring Cluster Physics with High-Resolution Sunyaev-Zel'dovich Effect Images and X-Ray Data: The Case of the Most X-Ray-Luminous Galaxy Cluster RX J1347-1145
T. Kitayama, E. Komatsu, N. Ota +5
Foreseeing the era of high spatial resolution measurements of the Sunyaev-Zel'dovich effect (SZE) in clusters of galaxies, we present a prototype analysis of this sort combined wit…
Modeling Pairwise Peculiar Velocity Distribution Function of Dark Matter from Halo Density Profiles
Takeshi Kuwabara, Atsushi Taruya, Yasushi Suto
We derive the pairwise peculiar velocity distribution function of dark matter particles applying the dark matter halo approach. Unlike the previous work, we do not assume a Gaussia…
Spin-triplet superconductivity due to antiferromagnetic spin-fluctuation in Sr_2RuO_4
Takeshi Kuwabara, Masao Ogata
A mechanism leading to the spin-triplet superconductivity is proposed based on the antiferromagnetic spin fluctuation. The effects of anisotropy in spin fluctuation on the Cooper p…