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Fig. 11.


FWHM of the Lyα line in the core (orange stars) and in the halo (blue points) plotted against the UV continuum slope of the host galaxy (calculated in H17). The larger symbols indicate the six S/NHALO >  10 objects. The Spearman rank correlation coefficients ρs and corresponding p0 values are indicated. See also Fig. A.3 for other relations between the Lyα line properties and the UV properties of the host galaxy.

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