Fig. 18 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. 18.

Frequency spectrum of the EE and BB power spectra for the region outside the P06 mask. To increase the signal‐to‐noise ratio, multiple values of ﹩l﹩ are averaged as indicated. Only statistical errors are shown. Negative values are not plotted. The frequency band combinations are given in Table 5. The thin red line running close to the ﹩l=2﹩ EE spectrum is the model in eq. (26). The dot‐dashed red line corresponds to eq. (25) evaluated for BB at ﹩l=2﹩.

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