Fig. 9.
Spectra extracted by RDI for planets d and e in 2019 compared with their ADI-extracted spectra from 2016 as reported in Zurlo et al. (2016). The 2016 and 2019 planet spectra are matched at 1.25 μm for easier comparison of their shapes. The shaded regions indicate the 1σ error ranges of the spectra. The wavelength range 1.37–1.45 μm, which is dominated by telluric lines, is not shown.
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