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Klaus Dolag

Researcher at Max Planck Society

Publications -  566
Citations -  78296

Klaus Dolag is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy cluster & Galaxy. The author has an hindex of 107, co-authored 516 publications receiving 73093 citations. Previous affiliations of Klaus Dolag include University of Padua & University of Bologna.

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The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

TL;DR: The Planck Sky Model (PSM) as mentioned in this paper is a parametric model for the generation of all-sky, few arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, in both intensity and polarisation.
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Connecting angular momentum and galactic dynamics: the complex interplay between spin, mass, and morphology

TL;DR: In this article, the authors used a hydrodynamical cosmological simulation taken from the set of Magneticum Pathfinder Simulations to understand the connection between the angular momentum of the dark matter halo and its galaxy.
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Planck Early Results XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

Peter A. R. Ade, +208 more
TL;DR: In this article, the authors presented precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-to-noise in the first Planck all-sky dataset.
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Planck early results - XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

Peter A. R. Ade, +252 more
TL;DR: In this paper, the authors presented precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-tonoise in the first Planck all-sky data set.
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Halo mass function: baryon impact, fitting formulae, and implications for cluster cosmology

TL;DR: In this article, a set of hydrodynamical and dark matter-only simulations were used to calibrate the halo mass function (HMF) of galaxy clusters, and an improved parametrization for spherical overdensity masses was proposed.