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J. Knoche

Researcher at Max Planck Society

Publications -  117
Citations -  23755

J. Knoche is an academic researcher from Max Planck Society. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 75, co-authored 117 publications receiving 22134 citations.

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Planck 2015 results: XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation

Peter A. R. Ade, +261 more
TL;DR: In this article, the authors used Planck data to detect the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) effect and the infrared emission from the galaxies that make up the cosmic infrared background (CIB).
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Planck intermediate results XVI. Profile likelihoods for cosmological parameters

Peter A. R. Ade, +234 more
TL;DR: In this paper, the authors explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Minuit), which allows a refinement of the CDM best-fit solution with respect to previously-released results, and the construction of frequentist confidence intervals using profile likelihoods.
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Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps

Peter A. R. Ade, +221 more
TL;DR: In this article, the polarization maps of three nearby star-forming filaments of moderate column density (NH about 1022 cm-2) were used to determine the intrinsic polarization properties of the filaments and provide insight into the structure of their magnetic field.
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Planck intermediate results. XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps

Peter A. R. Ade, +188 more
TL;DR: In this paper, the polarization maps of three nearby star forming filament of moderate column density (NH~10^22cm^-2): Musca, B211, and L1506 are presented.
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Planck intermediate results. XXIV. Constraints on variation of fundamental constants

P. A. R. Ade, +168 more
TL;DR: In this article, the authors show that the Planck data allow one to improve the constraint on the time variation of the fine structure constant at redshift by about a factor of 5 compared to WMAP data, as well as to break the degeneracy with the Hubble constant.