(2018) due to an increase in our determined stellar radius from both asteroseismology and Gaia parallaxes. Posteriors for the other parameters of our transit + stellar variability

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n a couple of recent papers we pointed out that gravitational mass, a primary magnitude, has intrinsic, essential, differences from inertial mass, a derived, secondary

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This value is consistent with other surveys for stellar companions around RV planet systems, but is much lower than the stellar companion fraction for transiting gas giant

For the giant planets recently identified, the deviations in the light curve can be substantial, although the specifics of the perturbations are dependent upon the radius of the

We outline that using a simple scalar as baseline model relies on the strong assumptions that the ensemble of comparison stars used to derive the di ff erential photometry has