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Caption: Figure 12.
Motion of the stellar secondary relative to the primary for the three CPM systems discussed in Section 7.1: (a) KOI-959; (b) KOI-1962; and (c) KOI-3214AB. In all plots, the filled circles represent observations taken earlier in our program and reported in Colton et al. (2021), the purple filled circles on the right marked “APO” indicate the new data appearing in Table 3, green diamonds are results from either Kraus et al. (2016), Wöllert & Brandner (2015), or Furlan et al. (2017), and red squares are measures from DR2 and DR3 of Gaia. The blue lines indicate the best-fit linear solution to the speckle data from our program.
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