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William T. Reach

Researcher at Universities Space Research Association

Publications -  545
Citations -  95523

William T. Reach is an academic researcher from Universities Space Research Association. The author has contributed to research in topics: Galaxy & Interstellar medium. The author has an hindex of 131, co-authored 535 publications receiving 90496 citations. Previous affiliations of William T. Reach include California Institute of Technology & Space Telescope Science Institute.

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Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization

Peter A. R. Ade, +178 more
TL;DR: In this article, the authors make use of the Planck 353 GHz I, Q, and U Stokes maps as dust templates, and cross-correlate them with the WMAP data at 12 frequencies from 23 to 353 GHz, over circular patches with 10 degree radius.
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Planck 2015 results. II. Low Frequency Instrument data processing

P. A. R. Ade, +236 more
TL;DR: An updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline is presented and it is demonstrated that the pipeline is self-consistent (principally based on simulations) and report all null tests.
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Dust in the Local Interstellar Wind

TL;DR: In this paper, the Ulysses and Galileo satellites of the mass spectrum and flux rate of interstellar dust within the heliosphere are combined with information about the density, composition, and relative flow speed and direction of interstellar gas in the cloud surrounding the solar system to derive an in situ value for the gas-to-dust mass ratio, $R_{g/d} = 94^{+46}_{-38}$.
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The Dust cloud around the White Dwarf G 29-38

TL;DR: The spectral energy distribution of the white dwarf G 29-38 with the camera (4.5 and 8 microns), photometer (24 microns, and spectrograph (5.5-14 microns) of the Spitzer Space Telescope was observed in this article.
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Planck 2015 results - XXVIII. The Planck Catalogue of Galactic cold clumps

Peter A. R. Ade, +268 more
TL;DR: The Planck Catalogue of Galactic Cold Clumps (PGCC) as discussed by the authors is an all-sky catalogue of Galactic cold clump candidates detected by Planck and contains 13,188 sources spread across the whole sky, i.e., from the Galactic plane to high latitudes, following the spatial distribution of the main molecular cloud complexes.