Fig. 41
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Inferred cosmological parameters (redshift-space f and AP parameters) for the four samples, together with linear bias b1, in the redshift bin [0.9,1.1]. As in Fig. 40, the absolute magnitude-limited sample, Mr − 5 log10 h < −20, contours in magenta are hardly seen as they are very similar and are below the magnitude-limited sample, HE < 22, contours in green.
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