activity
19932023
most citedHEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere

6k citations · 13.1k across the 91 of their papers we have counts for

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Showing 2009 · astro-ph.COShow all

6 papers · 2 filters

astro-ph.CO2009★ 39 cited

Lensing reconstruction from PLANCK sky maps: inhomogeneous noise

Duncan Hanson, Graca Rocha, Krzysztof Gorski

We discuss the effects of inhomogeneous sky-coverage on CMB lens reconstruction, focusing on application to the recently launched Planck satellite. We discuss the mean-field which…

astro-ph.CO2009★ 60 cited

Study of the Experimental Probe of Inflationary Cosmology (EPIC)-Intemediate Mission for NASA's Einstein Inflation Probe

James Bock, Abdullah Aljabri, Alex Amblard +35

Measurements of Cosmic Microwave Background (CMB) anisotropy have served as the best experimental probe of the early universe to date. The inflationary paradigm, inspired in part b…

astro-ph.CO2009★ 266 cited

Increasing evidence for hemispherical power asymmetry in the five-year WMAP data

J. Hoftuft, H. K. Eriksen, A. J. Banday +3

(Abridged)Motivated by the recent results of Hansen et al. (2008) concerning a noticeable hemispherical power asymmetry in the WMAP data on small angular scales, we revisit the dip…

astro-ph.CO2009★ 10 cited

Bayesian analysis of white noise levels in the 5-year WMAP data

N. E. Groeneboom, H. K. Eriksen, K. Gorski +3

We develop a new Bayesian method for estimating white noise levels in CMB sky maps, and apply this algorithm to the 5-year WMAP data. We assume that the amplitude of the noise RMS…

astro-ph.CO2009★ 41 cited

Bayesian component separation and CMB estimation for the 5-year WMAP temperature data

C. Dickinson, H. K. Eriksen, A. J. Banday +6

A well-tested and validated Gibbs sampling code, that performs component separation and CMB power spectrum estimation, was applied to the {\it WMAP} 5-yr data. Using a simple model…

astro-ph.CO2009★ 4 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…