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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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Proceedings ArticleDOI

BICEP Array: a multi-frequency degree-scale CMB polarimeter

Howard Hui, +77 more
TL;DR: The BICEP Array as mentioned in this paper is the newest multi-frequency instrument in the BiceP/Keck Array program, consisting of four 550 mm aperture refractive telescopes observing the polarization of the cosmic microwave background (CMB) at 30/40, 95, 150 and 220/270 GHz with over 30,000 detectors.
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Planck 2013 results. IX. HFI spectral response

Peter A. R. Ade, +273 more
TL;DR: In this article, the Planck High Frequency Instrument (HFI) spectral response was determined through a series of ground-based tests conducted with the HFI focal plane in a cryogenic environment prior to launch.
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Planck intermediate results - XXXIV. The magnetic field structure in the Rosette Nebula

Nabila Aghanim, +236 more
TL;DR: In this article, the magnetic field structure of the Rosette nebula was studied using the Planck intensity map and rotation measure (RM) data from a massive star-forming region in the Monoceros molecular cloud.
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Planck intermediate results. XVIII. The millimetre and sub-millimetre emission from planetary nebulae

Monique Arnaud, +206 more
TL;DR: In this paper, the amount of ionized gas and dust in a very young PN CRL618 has been estimated using the Planck multi-frequency measurements from radio through to far-infrared frequencies.
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Planck intermediate results. XXXIV. The magnetic field structure in the Rosette Nebula

Nabila Aghanim, +198 more
TL;DR: In this article, the magnetic field in the Rosette nebula is modeled as a uniform shell of swept-up ISM, which is assumed to evolve from an initially uniform configuration following the expansion of ionized gas and the formation of a shell.