The figure shows an N-body fit of a multiple-planet system discovered with Doppler surveys (Antonova et al., in prep). Many archival, unpublished RVs are available for such systems. An immediate objective of EXO-RESTART is to perform the first homogeneous dynamical modeling of high-precision Doppler and transit photometry data consistent with multiple-planet systems to reveal the current dynamical architecture.
We also aim to dynamically characterize TESS/Kepler TTVs multiple-planet systems like the TOI-2525 system (Trifonov et al. submitted) shown below.
