output
20022015
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing astro-ph.COShow all

41 papers · 1 filter

astro-ph.CO2013

Why a Windy Torus?

S. C. Gallagher, M. M. Abado, J. E. Everett +2

Mass ejection in the form of winds or jets appears to be as fundamental to quasar activity as accretion, and can be directly observed in many objects with broadened and blue-shifte…

astro-ph.CO201360 cited

The WiggleZ Dark Energy Survey: measuring the cosmic growth rate with the two-point galaxy correlation function

Carlos Contreras, Chris Blake, Gregory B. Poole +24

The growth history of large-scale structure in the Universe is a powerful probe of the cosmological model, including the nature of dark energy. We study the growth rate of cosmic s…

astro-ph.CO201314 cited

The structure of the merging RCS 231953+00 Supercluster at z ~ 0.9

A. J. Faloon, T. M. A. Webb, E. Ellingson +8

The RCS 2319+00 supercluster is a massive supercluster at z=0.9 comprising three optically selected, spectroscopically confirmed clusters separated by <3 Mpc on the plane of the sk…

astro-ph.CO2012178 cited

Super-luminous supernovae at redshifts of 2.05 and 3.90

Jeff Cooke, Mark Sullivan, Avishay Gal-Yam +6

A rare class of `super-luminous' supernovae that are about ten or more times more luminous at their peaks than other types of luminous supernovae has recently been found at low to…

astro-ph.CO20124 cited

Simulating Cosmic Reionization and the Radiation Backgrounds from the Epoch of Reionization

Paul R. Shapiro, Ilian T. Iliev, Garrelt Mellema +10

Large-scale reionization simulations are described which combine the results of cosmological N-body simulations that model the evolving density and velocity fields and identify the…

astro-ph.CO201233 cited

Non-Gaussianity from Axionic Curvaton

Masahiro Kawasaki, Takeshi Kobayashi, Fuminobu Takahashi

We study non-Gaussianity of density perturbations generated by an axionic curvaton, focusing on the case that the curvaton sits near the hilltop of the potential during inflation.…