摘要: NIST produces large-format, dual-polarization-sensitive detector arrays for a broad range of frequencies (30-1400 GHz). Such arrays enable a host of astrophysical measurements. Detectors optimized for cosmic microwave background o... 展开
| 作者 | Hubmayr, J. Austermann, J. Hilton, G. C. Ho, S. P. Irwin, K. D. Koopman, B. J. Li, D. McMahon, J. Munson, C. Niemack, M. D. Pappas, C. Schmitt, B. L. Beall, J. Simon, S. M. Staggs, S. T. Van Lanen, J. Wollack, E. J. Becker, D. Cho, H. Datta, R. Duff, S. M. Grace, E. Halverson, N. Henderson, S. W. | ||
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| 原报告号 | N160005955 | 总页数 | 5 |
| 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 | Bolometers Cosmic microwave background radiation Antenna feeds Superconductivity Polarimetry Receivers Cosmology Astrophysics Detection Telescopes Pixels | ||
