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Fig. 35
2D marginalized posterior distribution for w0 and wa for Planck+WP+BAO data. The contours are 68% and 95%, and the samples are colour-coded according to the value of H0. Independent flat priors of −3 <w0< − 0.3 and −2 <wa< 2 are assumed. Dashed grey lines show the cosmological constant solution w0 = − 1 and wa = 0.
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