scispace - formally typeset
N

N. A. Larsen

Researcher at University of Chicago

Publications -  13
Citations -  683

N. A. Larsen is an academic researcher from University of Chicago. The author has contributed to research in topics: Cosmic microwave background & South Pole Telescope. The author has an hindex of 8, co-authored 13 publications receiving 561 citations. Previous affiliations of N. A. Larsen include California Institute of Technology.

Papers
More filters
Journal ArticleDOI

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.
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.
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.
Journal ArticleDOI

BICEP2 / Keck Array XI: Beam Characterization and Temperature-to-Polarization Leakage in the BK15 Dataset

Keck Array, +77 more
TL;DR: In this article, a cosmological constraint from observations with the BICEP2 and Keck Array experiments up to and including the 2015 observing season (BK15) was presented, resulting in the deepest CMB polarization maps to date and a statistical sensitivity to the tensor-to-scalar ratio of $\sigma(r) = 0.0027 \pm 0.020$.