Heller, René Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;
Oshagh, M., Heller, R., & Dreizler, S. (2016). How eclipse time variations, eclipse duration variations and radial velocities can reveal S-type planets in close eclipsing binaries. Mon. Not. Roy. Astron. Soc., 466, 4683-4691. doi:10.1093/mnras/stw3313.