Improved Constraints on Cosmology and Foregrounds from BICEP2 and Keck Array Cosmic Microwave Background Data with Inclusion of 95 GHz BandP. A. R. Ade, K. L. Thompson, V. Buza et al.|Physical Review Letters|2016Cited by 675
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 and Keck array: upgrades and improved beam characterizationI. Buder, C. D. Sheehy, P. A. R. Ade et al.|Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE|2014Cited by 41
BICEP2/KECK ARRAY. VII. MATRIX BASED E/B SEPARATION APPLIED TO BICEP2 AND THE KECK ARRAYP. A. R. Ade, B. Steinbach, Zeeshan Ahmed et al.|The Astrophysical Journal|2016Cited by 24
Keck array and BICEP3: spectral characterization of 5000+ detectorsK. S. Karkare, R. Schwarz, P. A. R. Ade et al.|Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE|2014Cited by 12