S
Suzanne Aigrain
Researcher at University of Oxford
Publications - 359
Citations - 28631
Suzanne Aigrain is an academic researcher from University of Oxford. The author has contributed to research in topics: Planet & Exoplanet. The author has an hindex of 89, co-authored 348 publications receiving 25967 citations. Previous affiliations of Suzanne Aigrain include University of Exeter & European Space Research and Technology Centre.
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Mon-735: a new low-mass pre-main-sequence eclipsing binary in NGC 2264
Edward Gillen,Lynne A. Hillenbrand,John R. Stauffer,Suzanne Aigrain,Luisa Rebull,Ann Marie Cody +5 more
TL;DR: In this paper, a detached double-lined eclipsing binary (EB) member of the ∼3 Myr old NGC 2264 star-forming region, detected by Spitzer, is presented.
Planetary transit candidates in Corot-IRa01 field
Stefania Carpano,J. Cabrera,Roi Alonso,Pierre Barge,Suzanne Aigrain,J. M. Almenara,Pascal Bordé,François Bouchy,Ludmila Carone,Hans J. Deeg,R. de la Reza,Magali Deleuil,Rudolf Dvorak,Anders Erikson,F. Fressin,M. Fridlund,P. Gondoin,Tristan Guillot,A. P. Hatzes,Laurent Jorda,Helmut Lammer,A. Léger,A. Llebaria,Pierre Magain,C. Moutou,Aviv Ofir,Marc Ollivier,Eduardo Janot-Pacheco,Martin Paetzold,Frederic Pont,D. Queloz,Heike Rauer,Clara Régulo,S. Renner,D. Rouan,B. Samuel,Jean Schneider,Günther Wuchterl +37 more
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Quasi-periodic Gaussian processes for stellar activity: From physical to kernel parameters
TL;DR: In this paper , the authors compare the posterior distributions of the Gaussian Process (GP) hyperparameters to the input parameters of the spot model, and find that good coverage of rotation period and spot evolution time-scales is more important than the total number of points and noise characteristics govern the harmonic complexity.
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Exoplanet atmospheres with EChO: spectral retrievals using EChOSim
Joanna K. Barstow,Neil Bowles,Suzanne Aigrain,Leigh N. Fletcher,Patrick G. J. Irwin,R. Varley,Enzo Pascale +6 more
TL;DR: In this paper, the authors demonstrate the effectiveness of the Exoplanet Characterisation Observatory mission concept for constraining the atmospheric properties of hot and warm gas giants and super Earths.
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Accuracy of stellar parameters of exoplanet-host stars determined from asteroseismology
TL;DR: In this article, a linear nonadiabatic stability analysis was used to derive uncertainties on fundamental stellar parameters and analyse the effect of varying the number of considered modes for a given accuracy of oscillation frequency determination.