Prof Suzanne Aigrain: Publications

Stellar_flare_hits_HD_189733_b_(artist's_impression)

This artist's impression shows the hot Jupiter HD 189733b, as it passes in front of its parent star, as the latter is flaring, driving material away from the planet. The escaping atmosphere is seen silhouetted against the starlight. The surface of the star, which is around 80% the mass of the Sun, is based on observations of the Sun from NASA's Solar Dynamics Observatory.

Credit: NASA, ESA, L. Calçada, Solar Dynamics Observatory

Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades

(2017)

Authors:

TR White, BJS Pope, V Antoci, PI Pápics, C Aerts, DR Gies, K Gordon, D Huber, GH Schaefer, S Aigrain, S Albrecht, T Barclay, G Barentsen, PG Beck, TR Bedding, M Fredslund Andersen, F Grundahl, SB Howell, MJ Ireland, SJ Murphy, MB Nielsen, V Silva Aguirre, PG Tuthill

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Pinning down the mass of Kepler-10c: the importance of sampling and model comparison

(2017)

Authors:

Vinesh Rajpaul, Lars A Buchhave, Suzanne Aigrain

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A deeper view of the CoRoT-9 planetary system A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering

ASTRONOMY & ASTROPHYSICS 603 (2017) ARTN A43

Authors:

AS Bonomo, G Hebrard, SN Raymond, F Bouchy, AL des Etangs, P Borde, S Aigrain, J-M Almenara, R Alonso, J Cabrera, S Csizmadia, C Damiani, HJ Deeg, M Deleuil, RF Diaz, A Erikson, M Fridlund, D Gandolfi, E Guenther, T Guillot, A Hatzes, A Izidoro, C Lovis, C Moutou, M Ollivier, M Paetzold, H Rauer, D Rouan, A Santerne, J Schneider

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Inferring probabilistic stellar rotation periods using Gaussian processes

(2017)

Authors:

Ruth Angus, Timothy Morton, Suzanne Aigrain, Daniel Foreman-Mackey, Vinesh Rajpaul

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New low-mass eclipsing binary systems in Praesepe discovered by K2

(2017)

Authors:

Edward Gillen, Lynne A Hillenbrand, Trevor J David, Suzanne Aigrain, Luisa Rebull, John Stauffer, Ann Marie Cody, Didier Queloz

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Prof Suzanne Aigrain

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Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades

Authors:

Pinning down the mass of Kepler-10c: the importance of sampling and model comparison

Authors:

A deeper view of the CoRoT-9 planetary system A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering

Authors:

Inferring probabilistic stellar rotation periods using Gaussian processes

Authors:

New low-mass eclipsing binary systems in Praesepe discovered by K2

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Prof Suzanne Aigrain

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Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades

Authors:

Pinning down the mass of Kepler-10c: the importance of sampling and model comparison

Authors:

A deeper view of the CoRoT-9 planetary system A small non-zero eccentricity for CoRoT-9b likely generated by planet-planet scattering

Authors:

Inferring probabilistic stellar rotation periods using Gaussian processes

Authors:

New low-mass eclipsing binary systems in Praesepe discovered by K2

Authors: