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Cosmological Parameter Estimation: Method

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Figure 1: Angular power spectrum estimates of the CMB anisotropies in September 2003 ([7, 8, 9, 10, 11, 12, 13, 14, 15])
Figure 2: Comparison to the TOCO97 likelihood function for all approximation described in this section
Figure 3: Comparison between marginalisation and maximization estimation of confidence intervals in an extreme case

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