APA (7th ed.) Citation

Martin, D. V., Mazeh, T., & Fabrycky, D. C. (2015). No circumbinary planets transiting the tightest Kepler binaries – a possible fingerprint of a third star. Monthly notices of the Royal Astronomical Society, 453(4), 3554-3567. https://doi.org/10.1093/mnras/stv1870

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." Monthly Notices of the Royal Astronomical Society 453, no. 4 (2015): 3554-3567. https://doi.org/10.1093/mnras/stv1870.

MLA (9th ed.) Citation

Martin, David V., et al. "No Circumbinary Planets Transiting the Tightest Kepler Binaries – a Possible Fingerprint of a Third Star." Monthly Notices of the Royal Astronomical Society, vol. 453, no. 4, 2015, pp. 3554-3567, https://doi.org/10.1093/mnras/stv1870.