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BICEP2 and Keck Array: Upgrades and Improved Beam Characterization

I. Buder,P. A. R. Ade,Z. Ahmed,R. W. Aikin,K. D. Alexander,M. Amiri,D. Barkats,S. J. Benton,C. A. Bischoff,J. J. Bock,J. A. Bonetti,J. A. Brevik,E. Bullock,B. Burger,B. P. Crill,G. Davis,C. D. Dowell,L. Duband,J. P. Filippini,S. Fliescher,S. R. Golwala,M. S. Gordon,M. Halpern,M. Hasselfield,S. R. Hildebrandt,G. C. Hilton,V. V. Hristov,H. Hui,K. D. Irwin,K. S. Karkare,J. P. Kaufman,B. G. Keating,S. Kefeli,S. A. Kernasovskiy,J. M. Kovac,C. L. Kuo,E. M. Leitch,M. Lueker,P. Mason,K. G. Megerian,C. B. Netterfield,H. T. Nguyen,R. O'Brient,R. W. Ogburn,A. Orlando,C. Pryke,C. D. Reintsema,S. Richter,R. Schwarz,C. D. Sheehy,Z. K. Staniszewski,R. V. Sudiwala,G. P. Teply,K. L. Thompson,J. E. Tolan,A. D. Turner,A. G. Vieregg,A. C. Weber,D. V. Wiebe,P. Wilson,C. L. Wong,K. W. Yoon

Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE（2014）

Cited 34|Views72
Key words
Inflation,Gravitational waves,Cosmic microwave background,polarization,BICEP2,Keck Array
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