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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The photospheric abundances of active binaries I Detailed analysis of HD 113816 (IS Vir) and HD 119285 (V851 Cen)
TL;DR: In this article, high-resolution optical spectra of RS CVn stars HD 113816 (IS Vir) and HD 119285 (V851 Cen) are analyzed and their Na, Mg, Al, Si, Ca, Sc, Ti, Co and Ni contents determined.
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The K2 Bright Star Survey. I. Methodology and data release
Benjamin J. S. Pope,Timothy R. White,Timothy R. White,Timothy R. White,Will M. Farr,Will M. Farr,Jie Yu,Michael Greklek-McKeon,Daniel Huber,Conny Aerts,Conny Aerts,Conny Aerts,Suzanne Aigrain,Timothy R. Bedding,Timothy R. Bedding,Tabetha S. Boyajian,Orlagh Creevey,David W. Hogg +17 more
TL;DR: In this article, the unsaturated scattered-light halo is used to extract light curves from both normal and saturated stars, and the weights of a linear combination of pixel time series with respect to an objective function are optimized.
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One year of AU Mic with HARPS: I -- measuring the masses of the two transiting planets
N. Zicher,Oscar Barrag'an,Baptiste Klein,Suzanne Aigrain,James E. Owen,Davide Gandolfi,Anne-Marie Lagrange,L. M. Serrano,Laurel Kaye,Louise D. Nielsen,Vinesh Rajpaul,A. Grandjean,E. Goffo,Belinda A. Nicholson +13 more
TL;DR: In this paper , the authors used a multidimensional Gaussian Process framework to model the peak-to-peak activity-induced radial velocity (RV) variations of the AU Mic system.
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Erratum: Transit spectroscopy with JWST: systematics, star-spots and stitching
TL;DR: Barstow et al. as discussed by the authors presented the primary transit spectra of a 2RE rocky super-Earth with an Earth-like atmosphere, which is the case for the true Earth analogue.
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The GTC exoplanet transit spectroscopy survey VIII. Flat transmission spectrum for the warm gas giant WASP-80
Hannu Parviainen,Enric Palle,Guo Chen,Lisa Nortmann,Felipe Murgas,Grzegorz Nowak,Suzanne Aigrain,Alice S. Booth,Mantas Abazorius,Nicolas Iro +9 more
TL;DR: In this article, the authors used ground-based transmission spectroscopy to study the atmosphere of WASP-80b, a warm inflated gas giant with an equilibrium temperature of ∼$800~K, covering the spectral range from 520~to~910~nm.