Institution
University of British Columbia
Education•Vancouver, British Columbia, Canada•
About: University of British Columbia is a education organization based out in Vancouver, British Columbia, Canada. It is known for research contribution in the topics: Population & Poison control. The organization has 89939 authors who have published 209679 publications receiving 9226862 citations. The organization is also known as: UBC & The University of British Columbia.
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University of Kiel1, University of British Columbia2, University of Messina3, National Institutes of Health4, University of Freiburg5, University of Bern6, Kyoto University7, University of Siena8, University of Western Australia9, The Catholic University of America10, Goethe University Frankfurt11, University of Barcelona12, Copenhagen University Hospital13
TL;DR: These guidelines cover practical aspects of TMS in a clinical setting and lay out the general principles that apply to a standardized clinical examination of the fast-conducting corticomotor pathways with single-pulse TMS.
901 citations
TL;DR: Efforts to increase the frequency of the appropriateness of initial antimicrobial therapy must be central to efforts to reduce the mortality of patients with septic shock.
901 citations
TL;DR: The concept that superconductivity competes with other orders in cuprate superconductors has become increasingly apparent, but obtaining direct evidence with bulk-sensitive probes is challenging as discussed by the authors.
Abstract: The concept that superconductivity competes with other orders in cuprate superconductors has become increasingly apparent, but obtaining direct evidence with bulk-sensitive probes is challenging We have used resonant soft x-ray scattering to identify two-dimensional charge fluctuations with an incommensurate periodicity of ~32 lattice units in the copper-oxide planes of the superconductors (Y,Nd)Ba(2)Cu(3)O(6+)(x), with hole concentrations of 009 to 013 per planar Cu ion The intensity and correlation length of the fluctuation signal increase strongly upon cooling down to the superconducting transition temperature (T(c)); further cooling below T(c) abruptly reverses the divergence of the charge correlations In combination with earlier observations of a large gap in the spin excitation spectrum, these data indicate an incipient charge density wave instability that competes with superconductivity
899 citations
Swinburne University of Technology1, New York University2, University of Western Australia3, University of Queensland4, University of Copenhagen5, Australian Astronomical Observatory6, University of Sydney7, California Institute of Technology8, University of Waterloo9, University of Chicago10, Australia Telescope National Facility11, Carnegie Institution for Science12, Monash University, Clayton campus13, Australian National University14, University of British Columbia15, University of Toronto16
TL;DR: In this paper, the authors present measurements of the baryon acoustic peak at redshifts z = 0.44, 0.6 and 0.73 in the galaxy correlation function of the final dataset of the WiggleZ Dark Energy Survey.
Abstract: We present measurements of the baryon acoustic peak at redshifts z = 0.44, 0.6 and 0.73 in the galaxy correlation function of the final dataset of the WiggleZ Dark Energy Survey. We combine our correlation function with lower-redshift measurements from the 6-degree Field Galaxy Survey and Sloan Digital Sky Survey, producing a stacked survey correlation function in which the statistical significance of the detection of the baryon acoustic peak is 4.9-σ relative to a zero-baryon model with no peak. We fit cosmological models to this combined baryon acoustic oscillation (BAO) dataset comprising six distance-redshift data points, and compare the results to similar fits to the latest compilation of supernovae (SNe) and Cosmic Microwave Background (CMB) data. The BAO and SNe datasets produce consistent measurements of the equation-ofstate w of dark energy, when separately combined with the CMB, providing a powerful check for systematic errors in either of these distance probes. Combining all datasets we determine w = 1.03 ± 0.08 for a flat Universe, consistent with a cosmological constant model. Assuming dark energy is a cosmological constant and varying the spatial curvature, we find k = 0.004± 0.006.
898 citations
897 citations
Authors
Showing all 90682 results
| Name | H-index | Papers | Citations |
|---|---|---|---|
| Gordon H. Guyatt | 231 | 1620 | 228631 |
| John C. Morris | 183 | 1441 | 168413 |
| Douglas Scott | 178 | 1111 | 185229 |
| John R. Yates | 177 | 1036 | 129029 |
| Deborah J. Cook | 173 | 907 | 148928 |
| Richard A. Gibbs | 172 | 889 | 249708 |
| Evan E. Eichler | 170 | 567 | 150409 |
| James F. Sallis | 169 | 825 | 144836 |
| Michael Snyder | 169 | 840 | 130225 |
| Jiawei Han | 168 | 1233 | 143427 |
| Michael Kramer | 167 | 1713 | 127224 |
| Bruce L. Miller | 163 | 1153 | 115975 |
| Peter A. R. Ade | 162 | 1387 | 138051 |
| Marc W. Kirschner | 162 | 457 | 102145 |
| Kaj Blennow | 160 | 1845 | 116237 |