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

Stellar surface information from the Ca II H&K lines - II. Defining better activity proxies

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2024) stae2508

Authors:

M Cretignier, NC Hara, AGM Pietrow, Y Zhao, H Yu, X Dumusque, A Sozzetti, C Lovis, S Aigrain

More details from the publisher

More details

Stellar surface information from the Ca II H&K lines -- II. Defining better activity proxies

(2024)

Authors:

M Cretignier, NC Hara, AGM Pietrow, Y Zhao, H Yu, X Dumusque, A Sozzetti, C Lovis, S Aigrain

Details from ArXiV

A Gaussian process model for stellar activity in 2-D line profile time-series

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2024) stae2421-stae2421

Authors:

Haochuan Yu, Suzanne Aigrain, Baptiste Klein, Michael Cretignier, Florian Lienhard, Stephen J Roberts

More details from the publisher

Details from ORA

More details

A Gaussian process model for stellar activity in 2-D line profile time-series

(2024)

Authors:

Haochuan Yu, Suzanne Aigrain, Baptiste Klein, Michael Cretignier, Florian Lienhard, Stephen J Roberts

Details from ArXiV

Revisiting the dynamical masses of the transiting planets in the young AU Mic system: Potential AU Mic b inflation at ~20 Myr

Astronomy & Astrophysics EDP Sciences 689 (2024) a132

Authors:

M Mallorquín, VJS Béjar, N Lodieu, MR Zapatero Osorio, H Yu, A Suárez Mascareño, M Damasso, J Sanz-Forcada, I Ribas, A Reiners, A Quirrenbach, PJ Amado, JA Caballero, S Aigrain, O Barragán, S Dreizler, A Fernández-Martín, E Goffo, Th Henning, A Kaminski, B Klein, R Luque, D Montes, JC Morales, E Nagel, E Pallé, S Reffert, M Schlecker, A Schweitzer

More details from the publisher

More details

Prof Suzanne Aigrain

Research theme

Sub department

Stellar surface information from the Ca II H&K lines - II. Defining better activity proxies

Authors:

Stellar surface information from the Ca II H&K lines -- II. Defining better activity proxies

Authors:

A Gaussian process model for stellar activity in 2-D line profile time-series

Authors:

A Gaussian process model for stellar activity in 2-D line profile time-series

Authors:

Revisiting the dynamical masses of the transiting planets in the young AU Mic system: Potential AU Mic b inflation at ~20 Myr

Authors:

FIND US

CONTACT US

Prof Suzanne Aigrain

Research theme

Sub department

Research groups

Stellar surface information from the Ca II H&K lines - II. Defining better activity proxies

Authors:

Stellar surface information from the Ca II H&K lines -- II. Defining better activity proxies

Authors:

A Gaussian process model for stellar activity in 2-D line profile time-series

Authors:

A Gaussian process model for stellar activity in 2-D line profile time-series

Authors:

Revisiting the dynamical masses of the transiting planets in the young AU Mic system: Potential AU Mic b inflation at ~20 Myr

Authors: