activity
19972023
most citedPlanck 2013 results. XII. Component separation

293 citations · 1.2k across the 21 of their papers we have counts for

collaborators

21 papers

gr-qc2023★ 2 cited

Membrane Models as a Means of Propulsion in General Relativity: Super-Luminal Warp-Drive that Satisfies the Weak Energy Condition

Greg Huey

Presented are toy-models for sub-luminal and super-luminal warp-drives in 3+1 dimensions. The models are constructed in a chimeric manner - as different bulk space-times separated…

astro-ph.CO2013★ 293 cited

Planck 2013 results. XII. Component separation

Planck Collaboration, P. A. R. Ade, N. Aghanim +252

Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwav…

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-ph2008★ 26 cited

CMB likelihood approximation by a Gaussianized Blackwell-Rao estimator

Ø. Rudjord, N. E. Groeneboom, H. K. Eriksen +3

We introduce a new CMB temperature likelihood approximation called the Gaussianized Blackwell-Rao (GBR) estimator. This estimator is derived by transforming the observed marginal p…

astro-ph2008★ 38 cited

A Markov Chain Monte Carlo Algorithm for analysis of low signal-to-noise CMB data

J. B. Jewell, H. K. Eriksen, B. D. Wandelt +3

We present a new Monte Carlo Markov Chain algorithm for CMB analysis in the low signal-to-noise regime. This method builds on and complements the previously described CMB Gibbs sam…