QSO2 outflow characterization using data obtained with OSIRIS at the Gran Telescopio Canarias

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Fig. A.8.

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SDSS 1101+4004. Same figure caption as in Fig. A.1. The fact that NB, N2, and N3 show more compact spatial profiles than the seeing disk shows that this improved during the spectroscopic observations. Magenta squares are the same as in Fig. A.5.

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