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Institution

University of Victoria

EducationVictoria, British Columbia, Canada
About: University of Victoria is a education organization based out in Victoria, British Columbia, Canada. It is known for research contribution in the topics: Population & Galaxy. The organization has 14994 authors who have published 41051 publications receiving 1447972 citations. The organization is also known as: Victoria College.


Papers
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Journal ArticleDOI
Georges Aad1, T. Abajyan2, Brad Abbott3, Jalal Abdallah4  +2942 moreInstitutions (200)
TL;DR: In this article, the production properties and couplings of the recently discovered Higgs boson using the decays into boson pairs were measured using the complete pp collision data sample recorded by the ATLAS experiment at the CERN Large Hadron Collider at centre-of-mass energies of 7 TeV and 8 TeV, corresponding to an integrated luminosity of about 25/fb.

513 citations

Journal ArticleDOI
TL;DR: A mixture of 45 peptide standards, easily adaptable to common plasma proteomics work flows, was created to permit absolute quantitation of 45 endogenous proteins in human plasma trypsin digests, and this mixture of internal standards has many uses and can be applied to the characterization oftrypsin digestion kinetics and plasma protein expression profiling.

511 citations

Journal ArticleDOI
TL;DR: In this paper, the free-streaming of warm dark matter (WDM) from Lyman-α flux-power spectra was studied using hydrodynamical simulations.
Abstract: We present new measurements of the free-streaming of warm dark matter (WDM) from Lyman-α flux-power spectra. We use data from the medium resolution, intermediate redshift XQ-100 sample observed with the X-shooter spectrograph (z = 3 – 4.2) and the high-resolution, high-redshift sample used in Viel et al. (2013) obtained with the HIRES/MIKE spectrographs (z = 4.2 - 5.4). Based on further improved modelling of the dependence of the Lyman-α flux-power spectrum on the free-streaming of dark matter, cosmological parameters, as well as the thermal history of the intergalactic medium (IGM) with hydrodynamical simulations, we obtain the following limits, expressed as the equivalent mass of thermal relic WDM particles. The XQ-100 flux power spectrum alone gives a lower limit of 1.4 keV, the re-analysis of the HIRES/MIKE sample gives 4.1 keV while the combined analysis gives our best and significantly strengthened lower limit of 5.3 keV (all 2σ C.L.). The further improvement in the joint analysis is partly due to the fact that the two data sets have different degeneracies between astrophysical and cosmological parameters that are broken when the data sets are combined, and more importantly on chosen priors on the thermal evolution. These results all assume that the temperature evolution of the IGM can be modelled as a power law in redshift. Allowing for a non-smooth evolution of the temperature of the IGM with sudden temperature changes of up to 5000K reduces the lower limit for the combined analysis to 3.5 keV. A WDM with smaller thermal relic masses would require, however, a sudden temperature jump of 5000K or more in the narrow redshift interval z = 4.6 - 4.8, in disagreement with observations of the thermal history based on high-resolution resolution Lyman-α forest data and expectations for photo-heating and cooling in the low density IGM at these redshifts.

510 citations

Journal ArticleDOI
TL;DR: In this paper, an approach in which the target particle itself plays an active part now achieves this using a lower light intensity, which means that heat-sensitive targets such as viruses could be manipulated directly.
Abstract: Optical tweezers use the forces exerted by light to manipulate objects at the micrometre scale. An approach in which the target particle itself plays an active part now achieves this using a lower light intensity. This reduction means that heat-sensitive targets such as viruses could be manipulated directly.

509 citations

Journal ArticleDOI
TL;DR: The Canadian Earth System Model version 5 (CanESM5) as mentioned in this paper is a global model developed to simulate historical climate change and variability, to make centennial-scale projections of future climate, and to produce initialized seasonal and decadal predictions.
Abstract: . The Canadian Earth System Model version 5 (CanESM5) is a global model developed to simulate historical climate change and variability, to make centennial-scale projections of future climate, and to produce initialized seasonal and decadal predictions. This paper describes the model components and their coupling, as well as various aspects of model development, including tuning, optimization, and a reproducibility strategy. We also document the stability of the model using a long control simulation, quantify the model's ability to reproduce large-scale features of the historical climate, and evaluate the response of the model to external forcing. CanESM5 is comprised of three-dimensional atmosphere (T63 spectral resolution equivalent roughly to 2.8 ∘ ) and ocean (nominally 1 ∘ ) general circulation models, a sea-ice model, a land surface scheme, and explicit land and ocean carbon cycle models. The model features relatively coarse resolution and high throughput, which facilitates the production of large ensembles. CanESM5 has a notably higher equilibrium climate sensitivity (5.6 K) than its predecessor, CanESM2 (3.7 K), which we briefly discuss, along with simulated changes over the historical period. CanESM5 simulations contribute to the Coupled Model Intercomparison Project phase 6 (CMIP6) and will be employed for climate science and service applications in Canada.

509 citations


Authors

Showing all 15188 results

NameH-indexPapersCitations
Jie Zhang1784857221720
D. M. Strom1763167194314
Sw. Banerjee1461906124364
Robert J. Glynn14674888387
Manel Esteller14671396429
R. Kowalewski1431815135517
Paul Jackson141137293464
Mingshui Chen1411543125369
Ali Khademhosseini14088776430
Roger Jones138998114061
Tord Ekelof137121291105
L. Köpke13695081787
M. Morii1341664102074
Arnaud Ferrari134139287052
Richard Brenner133110887426
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
202379
2022348
20212,108
20202,200
20192,212
20181,926