Fig. 14 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. 14.

Polarization masks, in Galactic coordinates, are shown for the P02, P04, P06, and P10 cut levels. The cross‐hatched region along the Galactic plane, common to all polarization masks, shows the dust intensity cut. The P06 cut is outlined by the black curve. The masked sources are in violet. The north ecliptic pole (NEP), south ecliptic pole (SEP), and Galactic center (GC) are indicated.

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