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Fig. 6

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Gaussian-fitting resulting parameters for the Paβ line of GSC06214b. Left: correlations between intrinsic FWHM and the line peak location µ0, arrows represent an upper limit on the intrinsic FWHM. Right: correlations between the Paβ line flux and the line peak location µ0. The intrinsic FWHM is computed as the square root of the quadratic difference between the measured line FWHM and the LSF FWHM. The µ0 parameter is relative to the line expected wavelength in vacuum (1.2821578 µm).

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