Fig. 1: Orbital properties of the 70 cool giants.
From: An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i
A comparison of the derived orbital eccentricities from this work (y axis) versus the orbital periods (previously known) for our planetary-candidate sample. We use colour (legend) to depict the dynamical ‘temperature’ via the inferred absence/presence of TTVs.
