comm.) and the small sample statistics following the prescription in @Mawet2014.]{}

              Filter   $\rho$ (mas)   $\theta$ (deg)     $\Delta$mag
  ---------- -------- -------------- ----------------- ----------------
  Star 1       $K1$     5723$\pm$6    126.13$\pm$0.14   9.13$\pm$0.04
               $K2$     5723$\pm$6    126.14$\pm$0.14   9.26$\pm$0.03
  Star 2       $K1$     5499$\pm$6    123.70$\pm$0.14   10.91$\pm$0.03
               $K2$     5499$\pm$6    123.70$\pm$0.14   10.98$\pm$0.03
  [Bkgd]{}     $K1$    5035$\pm$10    319.84$\pm$0.17   14.55$\pm$0.10
  [star]{}     $K2$    5038$\pm$19    319.88$\pm$0.25   14.55$\pm$0.23

  : [Astrometry and photometry relative to the star of the point sources detected in the IRDIS field of view (Fig \[fig:irdisimfov\]).]{}[]{data-label="tab:photometryastrometry"}

We note in the IFS ADI image (bottom panel of Fig. \[fig:ifsim\]) a blob feature interior to the S2 spiral south of the star at $\sim$0.20$''$ at the $\sim$3 $\sigma$ level[, excluding the pixels at the same separation dominated by the disk features]{}. The feature is visible at the same location in all the individual IFS images and also in the images obtained after subtraction of a radial profile[, but]{} not in aggressive PCA and TLOCI reduced data (results not shown). We conclude that this feature is likely a residual from a disk feature.

Detection of point sources {#sec:pointsources}
==========================

The two first point sources listed in Table \[tab:photometryastrometry\] ([Stars 1 and 2]{}) were classified as a background stellar binary by @Grady2009. For the last point source 