Fig. 8
Dependencies between Lyα flux (upper panels) and EW (lower panels) and best fitted stellar masses (left panels) and dust AV (right panels). Typical error bars are marked in grey. ULIRGs are marked with a red ring. The very high EW object in the lower panels is LAE_COSMOS_94, see Sect. 4.3.2. No clear dependencies are seen, besides an apparent lack of objects at large Lyα fluxes and large extinctions.
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