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Constraints on Primordial Gravitational Waves Using <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mi>l</mml:mi><mml:mi>a</mml:mi><mml:mi>n</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:math>, WMAP, and New BICEP2/<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>K</mml:mi><mml:mi>e</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:math> Observations through the 2015 SeasonP. A. R. Ade, R. W. Ogburn, Zeeshan Ahmed et al.|Physical Review Letters|2018Cited by 499
BICEP2 / <i>Keck Array</i> IX: New bounds on anisotropies of CMB polarization rotation and implications for axionlike particles and primordial magnetic fieldsP. A. R. Ade, C. D. Sheehy, Zeeshan Ahmed et al.|Physical review. D/Physical review. D.|2017Cited by 61
BICEP3 performance overview and planned Keck Array upgradeJ. Grayson, J. E. Tolan, P. A. R. Ade et al.|Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE|2016Cited by 58