Fig. 11 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. 11.

Map of the correlation, Z, between the polarization angle derived from the polarization of starlight, and the polarization angle in the K band. In the regions of high K‐band polarization, the correlation is strong. The polarization directions are anticorrelated in the Orion‐Eridanus region near ﹩l=-165^{\circ }﹩, suggesting spatially distinguished regions of dust and synchrotron emission.

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