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Marion Dierickx

Researcher at Harvard University

Publications -  61
Citations -  1853

Marion Dierickx is an academic researcher from Harvard University. The author has contributed to research in topics: Cosmic microwave background & Stars. The author has an hindex of 17, co-authored 55 publications receiving 1241 citations. Previous affiliations of Marion Dierickx include Smithsonian Institution & Max Planck Society.

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Constraints on Primordial Gravitational Waves Using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season.

Peter A. R. Ade, +84 more
TL;DR: Results from an analysis of all data taken by the bicep2/Keck CMB polarization experiments up to and including the 2015 observing season are presented, showing the strongest constraints to date on primordial gravitational waves.
Journal ArticleDOI

Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season.

P. A. R. Ade, +91 more
TL;DR: In this paper, the authors present results from an analysis of all data taken by the BICEP2, Keck Array, and BiceP3 CMB polarization experiments up to and including the 2018 observing season.
Posted Content

CMB-S4: Forecasting Constraints on Primordial Gravitational Waves

TL;DR: Abazajian et al. as discussed by the authors developed a forecasting framework that includes a power-spectrum-based semi-analytic projection tool, targeted explicitly towards optimizing constraints on the tensor-to-scalar ratio, in the presence of Galactic foregrounds and gravitational lensing of the CMB.
Proceedings ArticleDOI

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

Howard Hui, +77 more
- 09 Jul 2018 - 
TL;DR: The Bicep Array as discussed by the authors is the latest multi-frequency instrument in the BICEp/Keck Array program, consisting of four 550mm 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.
Journal ArticleDOI

Predicted Extension of the Sagittarius Stream to the Milky Way Virial Radius

TL;DR: In this article, a model of the Sagittarius (Sgr) stream and resulting stellar stream is used to simulate the full infall trajectory of the Sgr progenitor from the time it first crossed the Milky Way virial radius 8 Gyr ago.