Fig. 4.
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Brδ, H2 (1–0) S(3) and [SiVI] blend (black) in the EMIR (top) and X-shooter (bottom) rest frame spectra. The blue line shows the predicted Brδ profile (+ continuum; see text). The results of subtracting Brδ from the original spectra are shown in red. The * marks the location of (or near) a possible artefact in the EMIR spectrum, responsible for the unexpectedly narrow [SiVI] peak.
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