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Fig. 10.
Spectra extracted by RDI for planet c compared with that of the L6 object, 2MASS J2148+4003 from Looper et al. (2008) and L7 object VHS J125601257 b from Gauza et al. (2015). The wavelength range 1.37–1.45 μm, which is dominated by telluric lines, is not shown.
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