Fig. 3
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Paß profiles, corrected from the atmospheric contribution and baseline subtracted (see Sects. 5.2 and 5.3). Each spectrum is labeled with the corresponding UT time at the start of the integration. First row: GQ Lup b lines for each epoch. Second and third rows: Same but for GSC06214b, with the addition of the individual OSIRIS lines from Bowler et al. (2011) (2010-07-09 epoch).
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