14.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR1.5k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR1.4k papers
- Humboldt-Universität zu BerlinDE1.4k papers
- Stockholm UniversitySE1.3k papers
- The University of TokyoJP1.3k papers
- University of OxfordGB1.3k papers
- National Institute for Subatomic PhysicsNL1.3k papers
- Columbia UniversityUS1.2k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR1.2k papers
- University of WuppertalDE1.2k papers
- The University of MelbourneAU1.2k papers
- University of GlasgowGB1.2k papers
59 papers · 1 filter
Observation of an extended VHE gamma-ray emission from MSH 15-52 with CANGAROO-III
T. Nakamori, H. kubo, T. Yoshida +2
We have observed the supernova remnant MSH 15-52 (G320.4-1.2), which contains the gamma-ray pulsar PSR B1509-58, using the CANGAROO-III imaging atmospheric Cherenkov telescope arra…
Effects of diversification among assets in an agent-based market model
F. Ghoulmié, M. Bartolozzi, C. P. Mellen +1
We extend to the multi-asset case the framework of a discrete time model of a single asset financial market developed in Ghoulmie et al (2005). In particular, we focus on adaptive…
CANGAROO-III Observations of the 2006 Outburst of PKS2155-304
III collaboration, Y. Sakamoto, K. Nishijima +3
We have used the CANGAROO-III imaging atmospheric Cherenkov telescopes to observe the high-frequency-peaked BL Lacertae (HBL) object PKS 2155-304 between 2006 July 28 (MJD 53944) a…
Applications of physical methods in high-frequency futures markets
M. Bartolozzi, C. Mellen, F. Chan +3
In the present work we demonstrate the application of different physical methods to high-frequency or tick-by-tick financial time series data. In particular, we calculate the Hurst…
HESS VHE Gamma-Ray Sources Without Identified Counterparts
HESS Collaboration, F. Aharonian
The detection of gamma rays in the very-high-energy (VHE) energy range (100 GeV--100 TeV) provides a direct view of the parent population of ultra-relativistic particles found in a…
Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei
The Pierre Auger Collaboration
Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival directions of the cosmic rays with the highest energies, which are correlated with the…
Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals
The LIGO Scientific Collaboration, B. Abbott
We report on the methods and results of the first dedicated search for gravitational waves emitted during the inspiral of compact binaries with spinning component bodies. We analyz…
Upper limit on the diffuse flux of UHE tau neutrinos from the Pierre Auger Observatory
The Pierre Auger Collaboration
The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau-neutrinos that interact in the Earth's crust. Tau leptons from charged-cur…
Implications for the Origin of GRB 070201 from LIGO Observations
LIGO Scientific Collaboration, K. Hurley
We analyzed the available LIGO data coincident with GRB 070201, a short duration hard spectrum gamma-ray burst whose electromagnetically determined sky position is coincident with…
Optimisation of sample thickness for THz-TDS measurements
W. Withayachumnankul, B. M. Fischer, D. Abbott
How thick should the sample be for a transmission THz-TDS measurement? Should the sample be as thick as possible? The answer is `no'. Although more thickness allows T-rays to inter…
Symmetries and Invariant Differential Pairings
Michael G. Eastwood
The purpose of this article is to motivate the study of invariant, and especially conformally invariant, differential pairings. Since a general theory is lacking, this work merely…
Upper Limits from HESS AGN Observations in 2005-2007
HESS Collaboration, F. Aharonian
AIMS: Very high energy (VHE; E>100 GeV) gamma-ray studies were performed for 18 active galactic nuclei (AGN) from a variety of AGN classes. METHODS: VHE observations of a sample of…
Science With The Australian Square Kilometre Array Pathfinder
Simon Johnston
The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive…
Risk, ambiguity and quantum decision theory
Riccardo Franco
In the present article we use the quantum formalism to describe the effects of risk and ambiguity in decision theory. The main idea is that the probabilities in the classic theory…
LIGO: The Laser Interferometer Gravitational-Wave Observatory
The LIGO Scientific Collaboration, B. Abbott
The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study gravitational waves of astrophysical origin. Direct detection of gravitational wa…
Exploring the High-Energy Cosmic Ray Spectrum with a Toy Model of Cosmic Ray Diffusion
Roger Clay, Roland M. Crocker
We introduce a static toy model of the cosmic ray (CR) universe in which cosmic ray propagation is taken to be diffusive and cosmic ray sources are distributed randomly with a dens…
Numerical removal of water-vapor effects from THz-TDS measurements
Withawat Withayachumnankul, Bernd M. Fischer, Samuel P. Mickan +1
One source of disturbance in a pulsed T-ray signal is attributed to ambient water vapor. Water molecules in the gas phase selectively absorb T-rays at discrete frequencies correspo…
D-branes, KK-theory and duality on noncommutative spaces
J. Brodzki, V. Mathai, J. Rosenberg +1
We present a new categorical classification framework for D-brane charges on noncommutative manifolds using methods of bivariant K-theory. We describe several applications includin…
Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7--3946 with deep H.E.S.S. observations
S Collaboration, D. Berge, F. Aharonian +5
The shell-type supernova remnant RX J1713.7--3946 was observed during three years with the H.E.S.S. Cherenkov telescope system. The first observation campaign in 2003 yielded the f…
Twisted mass QCD at finite temperature
E. -M. Ilgenfritz, M. Müller-Preußker, M. Petschlies +5
We discuss the use of Wilson fermions with twisted mass for simulations of QCD thermodynamics. As a prerequisite for a future analysis of the finite-temperature transition making u…
A Joint Search for Gravitational Wave Bursts with AURIGA and LIGO
AURIGA Collaboration, LIGO Scientific Collaboration, L. Baggio et al
The first simultaneous operation of the AURIGA detector and the LIGO observatory was an opportunity to explore real data, joint analysis methods between two very different types of…
The Landau gauge gluon and ghost propagators in 4D SU(3) gluodynamics in large lattice volumes
I. L. Bogolubsky, E. -M. Ilgenfritz, M. Müller-Preussker +1
We present recent results of the Landau gauge gluon and ghost propagators in SU(3) pure gauge theory at Wilson β=5.7 for lattice sizes up to 80^4 corresponding to physical volumes…
Marking up lattice QCD configurations and ensembles
P. Coddington, B. Joo, C. M. Maynard +2
QCDml is an XML-based markup language designed for sharing QCD configurations and ensembles world-wide via the International Lattice Data Grid (ILDG). Based on the latest release,…
New constraints on the Mid-IR EBL from the HESS discovery of VHE gamma rays from 1ES 0229+200
HESS Collaboration, F. Aharonian
AIMS: To investigate the very high energy (VHE: >100 GeV) gamma-ray emission from the high-frequency peaked BL Lac 1ES 0229+200. METHODS: Observations of 1ES 0229+200 at energies a…