APA (7th ed.) Citation

Martin, D. V., Mazeh, T., & Fabrycky, D. C. (2015, August 14). No circumbinary planets transiting the tightest Kepler binaries - a possible fingerprint of a third star. arXiv.org. https://doi.org/10.48550/arxiv.1505.05749

Chicago Style (17th ed.) Citation

Martin, David V., Tsevi Mazeh, and Daniel C. Fabrycky. "No Circumbinary Planets Transiting the Tightest Kepler Binaries - a Possible Fingerprint of a Third Star." ArXiv.org 14 Aug. 2015. https://doi.org/10.48550/arxiv.1505.05749.

MLA (9th ed.) Citation

Martin, David V., et al. "No Circumbinary Planets Transiting the Tightest Kepler Binaries - a Possible Fingerprint of a Third Star." ArXiv.org, 14 Aug. 2015, https://doi.org/10.48550/arxiv.1505.05749.