Fig. 15

Near-infrared excess E(Ks−L′)for the primary and secondary components of each binary with individual component photometry. Red filled circles and blue filled diamonds are binaries with accreting primaries and secondaries. Targets to the right and above the dotted lines have significant near-IR excess, indicating the presence of inner disk material. A typical error bar, dominated by the systematic uncertainty of ~0.2 mag, is indicated in the upper left.
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