Fig. 1
Top: spectrum extracted between 0
15...03. The green line describes the Gaussian fit to the C iv emission, the red curve includes the H2 contamination. Bottom: C iv and H2 flux along the jet axis summed between –400 to 0 km s-1 for the C iv emission and –80 to 0 km s-1 for the H2 lines in our FUV spectrum. Included is [O iii] λ5007 emission seen in short G430L spectra.
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