Fig. 22 from Three‐Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis

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Three‐Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis

Authors: L. Page, G. Hinshaw, E. Komatsu, M. R. Nolta, D. N. Spergel, C. L. Bennett, C. Barnes, R. Bean, O. Doré, J. Dunkley, M. Halpern, R. S. Hill, N. Jarosik, A. Kogut, M. Limon, S. S. Meyer, N. Odegard, H. V. Peiris, G. S. Tucker, L. Verde, J. L. Weiland, E. Wollack, and E. L. Wright

Page et al. 2007 The Astrophysical Journal Supplement Series 170 335.

Provider: AAS Journals

Caption: Fig. 22.

EE spectrum at ﹩l> 40﹩ for all measurements of the CMB polarization. The curve is the best‐fit EE spectrum. Note that the y‐axis has only one power of ﹩l﹩. The black boxes are the WMAP data; the triangles are the BOOMERANG data; the squares are the DASI data; the diamonds are the CBI data; and the asterisk (*) is the CAPMAP data. The WMAP data are the QVW combination. For the first point, the cleaned value is used. For other values, the raw values are used. The data are given in Table 8.

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