Fig. 11
1–4 μm spectral energy distribution of HD 95086 b (SPHERE IFS JIFS, HIFS, and IRDIS K1 and K2 photometric datasets in green, GPI H and K1 photometric datasets in purple, GPI low-resolution K1 spectrum in black, and NaCo L ′ photometricdatset in red.) compared to that of young and/or dusty L7-L7.5 dwarfs and companions (dark red) younger than the field.
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