Image Details
Caption: Figure 16.
Fitting output for a mock astrometric dataset generated using BSPL_PhotAstrom_noPar_EllOrbs_Param1 and the parameters displayed in Table 6. We present a fit for the R.A. component in this figure. (Left) Best fit with linear orbital motion. (Center) Best fit with circular orbital motion. (Right) Best fit with elliptical orbital motion.
© 2026. The Author(s). Published by the American Astronomical Society.