Fig. 12
H i column density as a function of the integrated flux in the narrow Lyα emission peak (left), the quasar absolute luminosity as a function of the Lyα emission luminosity (center), and the deconvolved FHWM from a Gaussian fit to the narrow Lyα emission peak (right) as a function of the Lyα emission luminosity. DLAs that are part of the statistical sample are shaded in cyan.
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