Image Details
Caption: Fig. 10.
The 68% and 90% confidence intervals for β and ﹩\Omega _{m}﹩, where (a) ﹩\Omega _{\Lambda }=0﹩ (no cosmological constant) and (b) ﹩\Omega _{\Lambda }=1-\Omega _{m}﹩ (spatially flat universe)
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