Fig. 13 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. 13.

Constraints on the geometry of the universe:﹩\Omega _{m}- \Omega _{\Lambda }﹩ plane. Two‐dimensional likelihood surface for various combinations of data: WMAP (upper left); WMAPext (upper right); WMAPext+HST Key Project (supernova data [Riess et al. 1998, 2001] are shown but not used in the likelihood in this part of the panel) (lower left); WMAPext+HST Key Project+supernova (lower right).

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