PAPPA: Primordial anisotropy polarization pathfinder array

被引:13
作者
Kogut, A. [1 ]
Chuss, D. T.
Fixsen, D.
Hinshaw, G. F.
Limon, M.
Moseley, S. H.
Phillips, N.
Sharp, E.
Wollack, E. J.
U-Yen, K.
Cao, N.
Stevenson, T.
Hsieh, W.
Devlin, M.
Dicker, S.
Semisch, C.
Irwin, K.
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Sci Syst & Applicat Inc, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Global Sci & Technol, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] MEI Technol, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[5] Univ Penn, Philadelphia, PA 19104 USA
[6] Natl Inst Stand & Technol, Boulder, CO USA
基金
美国国家航空航天局;
关键词
cosmology; cosmic microwave background; polarization; instrumentation;
D O I
10.1016/j.newar.2006.09.024
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The primordial anisotropy polarization pathfinder array (PAPPA) is a balloon-based instrument to measure the polarization of the cosmic microwave background and search for the signal from gravity waves excited during an inflationary epoch in the early universe. PAPPA will survey a 20 x 20 patch at the North Celestial Pole using 32 pixels in 3 passbands centered at 89, 212, and 302 GHz. Each pixel uses MEMS switches in a superconducting microstrip transmission line to combine the phase modulation techniques used in radio astronomy with the sensitivity of transition-edge superconducting bolometers. Each switched circuit modulates the incident polarization on a single detector, allowing nearly instantaneous characterization of the Stokes I, Q, and U parameters. We describe the instrument design and status. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码:1009 / 1014
页数:6
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