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D. L. Harrison

Researcher at University of Cambridge

Publications -  170
Citations -  82147

D. L. Harrison is an academic researcher from University of Cambridge. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 112, co-authored 170 publications receiving 77713 citations.

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Overview of products and scientific results

R. Adam, +354 more
TL;DR: The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submillimetre sky continuously between 12~August 2009 and 23~October 2013 as discussed by the authors.
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Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope

Peter A. R. Ade, +195 more
TL;DR: In this article, the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with the Russian-Turkish 1.5m telescope (RTT150) are presented.
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Planck 2013 results. III. LFI systematic uncertainties

P. A. R. Ade, +221 more
TL;DR: In this article, the authors present the current accounting of systematic effect uncertainties for the Low Frequency Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results, showing the robustness and consistency of our data set, especially for polarization analysis.
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Planck 2013 results. IV. Low Frequency Instrument beams and window functions

Nabila Aghanim, +260 more
TL;DR: In this paper, the beam normalization and beam window functions for the Planck Low Frequency Instrument (LFI) were characterized and the uncertainties in the beam window function were analyzed.
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Planck intermediate results: XLIII. Spectral energy distribution of dust in clusters of galaxies

R. Adam, +249 more
TL;DR: In this article, the spectral energy distribution (SED) of the infrared spectrum of thermal dust emission in clusters of galaxies was obtained by using a stacking approach for a sample of several hundred objects from the Planck cluster sample; this procedure averaged out fluctuations from the IR sky, allowing to reach a significant detection of the faint cluster contribution.