References

References#

[FM16]

Daniel Foreman-Mackey. Corner.py: scatterplot matrices in python. The Journal of Open Source Software, 1(2):24, jun 2016. URL: https://doi.org/10.21105/joss.00024, doi:10.21105/joss.00024.

[ForemanMackeyHoggLangGoodman13]

D. Foreman-Mackey, D. W. Hogg, D. Lang, and J. Goodman. Emcee: the mcmc hammer. PASP, 125:306–312, 2013. arXiv:1202.3665, doi:10.1086/670067.

[HjorthAlbrechtHirano+21]

Maria Hjorth, Simon Albrecht, Teruyuki Hirano, Joshua N. Winn, Rebekah I. Dawson, J. J. Zanazzi, Emil Knudstrup, and Bun'ei Sato. A backward-spinning star with two coplanar planets. Proceedings of the National Academy of Science, 118(8):e2017418118, February 2021. arXiv:2102.07677, doi:10.1073/pnas.2017418118.

[LoudenWinnPetigura+21]

Emma M. Louden, Joshua N. Winn, Erik A. Petigura, Howard Isaacson, Andrew W. Howard, Kento Masuda, Simon Albrecht, and Molly R. Kosiarek. Hot Stars with Kepler Planets Have High Obliquities. \aj , 161(2):68, February 2021. arXiv:2012.00776, doi:10.3847/1538-3881/abcebd.

[MasudaWinn20]

Kento Masuda and Joshua N. Winn. On the Inference of a Star's Inclination Angle from its Rotation Velocity and Projected Rotation Velocity. \aj , 159(3):81, March 2020. arXiv:2001.04973, doi:10.3847/1538-3881/ab65be.

[McQuillanAigrainMazeh13]

A. McQuillan, S. Aigrain, and T. Mazeh. Measuring the rotation period distribution of field M dwarfs with Kepler. \mnras , 432(2):1203–1216, June 2013. arXiv:1303.6787, doi:10.1093/mnras/stt536.