摘要: Future arcminute resolution polarization data from ground-based Cosmic Microwave Background (CMB) observations can be used to estimate the contribution to the temperature power spectrum from the primary anisotropies and to uncover... 展开
作者 | Calabrese, E. Hlozek, R. Louis, T. McMahon, J. Moodley, K. Newburgh, L. Niemack, M. D. Page, L. A. Partridge, B. Sehgal, N. Sievers, J. L. Spergel, D. N. Battaglia, N. Staggs, S. T. Switzer, E. R. Trac, H. Wollack, E. J. Bond, J. R. De Bernardis, F. Devlin, M. J. Hajian, A. Henderson, S. Hil, J. C. Kosowsky, A. | ||
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原报告号 | N160001363 | 总页数 | 22 |
主办者 | National Aeronautics and Space Administration | ||
报告分类号 | [ 54C - Astrophysics] | ||
报告类别/文献类型 | DE / NTIS科技报告 | ||
关键词 | Cosmic microwave background radiation Temperature measurement Galactic clusters Background radiation Power spectra Cosmology Precision Spectra Kinematics Multipoles Anisotropy |