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S. R. Hildebrandt

Researcher at California Institute of Technology

Publications -  186
Citations -  68142

S. R. Hildebrandt is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 110, co-authored 184 publications receiving 61965 citations. Previous affiliations of S. R. Hildebrandt include Joseph Fourier University & Spanish National Research Council.

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Planck 2013 results. XIX. The integrated Sachs-Wolfe effect

Peter A. R. Ade, +311 more
TL;DR: In this paper, the authors presented the detection of the integrated Sachs-Wolfe (ISW) effect, that is, the correlation between the CMB and large-scale evolving gravitational potentials.
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BICEP2 / Keck Array V: Measurements of B-mode Polarization at Degree Angular Scales and 150 GHz by the Keck Array

TL;DR: In this paper, the authors report results from the 2012 and 2013 observing seasons, during which the Keck Array consisted of five receivers all operating in the same (150 GHz) frequency band and observing field as BICEP2.
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Planck Intermediate Results. IX. Detection of the Galactic haze with Planck

Peter A. R. Ade, +182 more
TL;DR: In this paper, the authors identify and characterize the emission from the Galactic "haze" at microwave wavelengths, which is a distinct component of diffuse Galactic emission, roughly centered on the Galactic centre, and extends to |b| ~35 deg in Galactic latitude and |l| ~15 deg in longitude.
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Planck Intermediate Results. IX. Detection of the Galactic haze with Planck

Peter A. R. Ade, +230 more
TL;DR: Using precise full-sky observations from Planck, and applying several methods of component separation, the authors of as discussed by the authors identify and characterise the emission from the Galactic haze at microwave wavelengths.
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Planck intermediate results XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust

R. Adam, +259 more
TL;DR: The role of the magnetic field in the formation of the filamentary structures observed in the interstellar medium (ISM) is a debated topic owing to the paucity of relevant observations needed to test existing models as discussed by the authors.