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Fig. 4


(Li)NLTE vs. [3.4]–[22] for the sample stars of Rebull et al. (2015). The vertical line at [3.4]–[22] = 0 indicates the photospheric locus. The blue points denote sources identified with IR excess by Rebull et al. (2015), while the black ones are for these with no obvious IR excess. The red star is our target.

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