Fig. 5
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Disk brightness in scattered light vs. near-IR excess. The polarized-to-stellar light contrast for the targets of this work and benchmark sample (see Sect. 3.3) is compared with the near-IR excess from the SED (see Appendix A). The spline fit is performed on all sources except non-detections and targets with local shadows (see Sect. 5.1). Target numbering refers to Table 1.
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