Using multi-transit systems to find stellar and planetary masses
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Using multi-transit systems to find stellar and planetary masses
Model-Independent Stellar and Planetary Masses from Multi-Transiting Exoplanetary Systems
http://arxiv.org/abs/1211.4028
Using planets near mean-motion resonances to obtain dynamical stellar and planetary masses. They apply the method to Kepler-18 c,d.
http://arxiv.org/abs/1211.4028
Using planets near mean-motion resonances to obtain dynamical stellar and planetary masses. They apply the method to Kepler-18 c,d.
Lazarus- dK star

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