Fig. 3 from First‐Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters

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First‐Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters

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

Spergel et al. 2003 The Astrophysical Journal Supplement Series 148 175.

Provider: AAS Journals

Caption: Fig. 3.

Contribution to ﹩2\mathrm{ln}\,\mathstrut{\cal L} ﹩ per multipole binned at ﹩\Delta \ell =15﹩. The excess ﹩\chi ^{2}﹩ comes primarily from three regions, one around ﹩\ell \sim 120﹩, one around ﹩\ell \sim 200﹩, and the other around ﹩\ell \sim 340﹩.

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