Fig. 28 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. 28.

Correlation coefficients of the Fisher matrices. The diamonds are derived from 100,000 Monte Carlo simulations, while the solid lines are the analytical formulae in the noise‐dominated regime. In the simulations, the B mode is noise only, while the E mode has some signals at low l from reionization.

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