activity
20042009
most citedThe Origin of the Universe as Revealed Through the Polarization of the Cosmic Microwave Background

15 citations · 29 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.CO20094 cited

Observing the Evolution of the Universe

James Aguirre, Alexandre Amblard, Amjad Ashoorioon +172

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the univers…

astro-ph.CO200915 cited

The Origin of the Universe as Revealed Through the Polarization of the Cosmic Microwave Background

S. Dodelson, R. Easther, S. Hanany +61

Modern cosmology has sharpened questions posed for millennia about the origin of our cosmic habitat. The age-old questions have been transformed into two pressing issues primed for…

astro-ph200810 cited

Covariance of dark energy parameters and sound speed constraints from large HI surveys

A. Torres-Rodriguez, C. M. Cress, K. Moodley

An interesting probe of the nature of dark energy is the measure of its sound speed, . We review the significance for constraining sound speed models of dark energy using larg…

astro-ph2005

Measuring the geometry of the Universe in the presence of isocurvature modes

J. Dunkley, M. Bucher, P. G. Ferreira +2

The Cosmic Microwave Background (CMB) anisotropy constrains the geometry of the Universe because the positions of the acoustic peaks of the angular power spectrum depend strongly o…

astro-ph2004

Constraints on isocurvature models from the WMAP first-year data

K. Moodley, M. Bucher, J. Dunkley +2

We investigate the constraints imposed by the first-year WMAP CMB data extended to higher multipole by data from ACBAR, BOOMERANG, CBI and the VSA and by the LSS data from the 2dF…

astro-ph2004

Fast and reliable MCMC for cosmological parameter estimation

Joanna Dunkley, Martin Bucher, Pedro G. Ferreira +2

Markov Chain Monte Carlo (MCMC) techniques are now widely used for cosmological parameter estimation. Chains are generated to sample the posterior probability distribution obtained…