GRB 031203: Comparison between weak emission line profiles in a spectrum integrating over the central 6 × 5 spaxels of the galaxy center (left column) and the same lines in an X-shooter spectrum presented in Guseva et al. (2011), Watson et al. (2011). The FLAMES spectra have been smoothed with a Gaussian kernel of 5 pixels in the spectral direction. Gray regions indicate contamination by residuals of atmospheric lines. For [N II] λ 6585 we fit a combination between a narrow and broad component based on the X-shooter spectrum using the same parameters to fit the line in the FLAMES spectrum.