Fig. 6
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IFS observations. Top: YJH-band images made from collapsing the IFS spectra and the locations from which the planet and disk spectra were extracted. Bottom: IFS Spectra of the b and c planets along with spectra of this dust ring at three locations. The planet spectra are similar to each other, and clearly different from the disk spectra. The region contaminated by telluric absorptions around 1.4 μ is grayed out.
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