American Astronomical Society, Astrophysical Journal Letters, 1(792), p. L22, 2014
DOI: 10.1088/2041-8205/792/1/l22
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We report the detection of a faint pointlike feature possibly related to ongoing planet-formation in the disk of the transition disk star HD 169142. The pointlike feature has a $Δ$mag(L)$∼$6.4, at a separation of $∼$0.11" and PA$∼$0$^{∘}$. Given its lack of an H or K$_{S}$ counterpart despite its relative brightness, this candidate cannot be explained by purely photospheric emission and must be a disk feature heated by an as yet unknown source. Its extremely red colors make it highly unlikely to be a background object, but future multi-wavelength followup is necessary for confirmation and characterization of this feature. ; Comment: Accepted to ApJ Letters, see also Reggiani et al. 2014