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

Written by exoplanetology | Published 2024/05/25
Tech Story Tags: kic-9851944 | kic-9851944-eclipsing-binary | eclipsing-binary | f-stars | tess-space-missions | kepler-space-missions | oscillations | mesa-evolutionary-code

TLDRStars that are both pulsating and eclipsing offer an important opportunity to better understand many of the physical phenomena that occur in stars.via the TL;DR App

This paper is available on arxiv under CC 4.0 license.

Authors:

(1) Z. Jennings, Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK (E-mail: z.jennings@keele.ac.uk);

(2) J. Southworth, Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK;

(3) K. Pavlovski, Department of Physics, Faculty of Science, University of Zagreb, 10000 Zagreb, Croatia;

(4) T. Van Reeth, Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium.

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APPENDIX A: EPHEMERIS DETERMINATION

This appendix presents the results from the preliminary JKTEBOP analaysis as well as times of primary minimum and fitted values calculated in section 3.


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Published by HackerNoon on 2024/05/25