Physical properties of the eclipsing binary KIC 9851944: Appendix A: Ephemeris Determination

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Physical properties of the eclipsing binary KIC 9851944: Appendix A: Ephemeris Determination
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Stars that are both pulsating and eclipsing offer an important opportunity to better understand many of the physical phenomena that occur in stars.

This paper is available on arxiv under CC 4.0 license. Authors: Z. Jennings, Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK ; J. Southworth, Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK; K. Pavlovski, Department of Physics, Faculty of Science, University of Zagreb, 10000 Zagreb, Croatia; T. Van Reeth, Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium.

Southworth, Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK; K. Pavlovski, Department of Physics, Faculty of Science, University of Zagreb, 10000 Zagreb, Croatia; T. Van Reeth, Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium.

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