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Ahmed Soliman

Researcher at University of Connecticut

Publications -  75
Citations -  1314

Ahmed Soliman is an academic researcher from University of Connecticut. The author has contributed to research in topics: Cosmic microwave background & Antenna (radio). The author has an hindex of 11, co-authored 64 publications receiving 798 citations. Previous affiliations of Ahmed Soliman include University of British Columbia & California Institute of Technology.

Papers
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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.
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.
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.
Proceedings ArticleDOI

Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole

TL;DR: The Bicep/Keck Array (BK) program targets the degree angular scales, where the power from primordial B-mode polarization is expected to peak, with ever increasing sensitivity and has published the most stringent constraints on inflation to date as discussed by the authors.