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VLT spectroscopy of the z=4.11 Radio Galaxy TN J1338-1942

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Figure

Fig. 1. 4.85 GHz VLA radio contours overlaid on a Keck K−band im- im-age. The cross indicates the position of the likely radio core at 8.5 GHz, which appears offset from the galaxy by 1
Fig. 3. Two dimensional FORS1 spectrum of the Lyα region. Note the strong, 1400 km s −1 wide depression in the blue half.
Fig. 4. Part of the spectrum around the Ly α line. The solid line is the model consisting of a Gaussian emission profile (dashed line) and a Voigt absorption profile with the indicated parameters.

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