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F. K. Hansen

Researcher at University of Rome Tor Vergata

Publications -  63
Citations -  12553

F. K. Hansen is an academic researcher from University of Rome Tor Vergata. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 42, co-authored 63 publications receiving 11944 citations. Previous affiliations of F. K. Hansen include Max Planck Society.

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HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere

TL;DR: The Hierarchical Equal Area iso-Latitude Pixelization (HEALPix) as discussed by the authors is a data structure with an associated library of computational algorithms and visualization software that supports fast scientific applications executable directly on very large volumes of astronomical data and large area surveys in the form of discretized spherical maps.
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Asymmetries in the Cosmic Microwave Background Anisotropy Field

TL;DR: In this paper, the power spectrum and N-point correlation functions of the Wilkinson Microwave Anisotropy Probe (WMAP) first-year data were used to measure the amplitudes of the large-scale fluctuations on opposing hemispheres and study the ratio of the two amplitudes.
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Asymmetries in the CMB anisotropy field

TL;DR: In this paper, two independent but complementary statistical analyses of the WMAP first-year data, based on the power spectrum and N-point correlation functions, are presented. But the results are stable with respect to the choice of Galactic cut and also with respect with the frequency band.
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Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources

P. A. R. Ade, +272 more
TL;DR: In this paper, the authors describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev-Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations.
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Planck Early Results: The Planck mission

P. A. R. Ade, +271 more
TL;DR: The European Space Agency's Planck satellite was launched on 14 May 2009, and has been surveying the sky stably and continuously since 13 August 2009 as discussed by the authors, and it will continue to gather scientific data until the end of its cryogenic lifetime.