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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Journal ArticleDOI
Hubble Space Telescope transmission spectroscopy of the exoplanet HD 189733b: high‐altitude atmospheric haze in the optical and near‐ultraviolet with STIS
David K. Sing,Frederic Pont,Suzanne Aigrain,D. Charbonneau,Jean-Michel Desert,Neale P. Gibson,R. L. Gilliland,Wolfgang Hayek,Gregory W. Henry,Heather A. Knutson,A. Lecavelier des Etangs,Tsevi Mazeh,Avi Shporer,Avi Shporer +13 more
TL;DR: In this article, the authors used time series spectra obtained during two transit events to determine the wavelength dependence of the planetary radius and measure the exoplanet's atmospheric transmission spectrum for the first time over this wavelength range.
Journal ArticleDOI
3.6 and 4.5 μm Phase Curves and Evidence for Non-equilibrium Chemistry in the Atmosphere of Extrasolar Planet HD 189733b
Heather Knutson,Nikole K. Lewis,Jonathan J. Fortney,Adam Burrows,Adam P. Showman,Nicolas B. Cowan,Eric Agol,Suzanne Aigrain,David Charbonneau,Drake Deming,Jean-Michel Desert,Gregory W. Henry,Jonathan Langton,Gregory Laughlin +13 more
TL;DR: In this article, the infrared phase variations of the hot Jupiter HD 189733b obtained in the 3.6 and 4.5 μm bands using the Spitzer Space Telescope were used to characterize the exoplanet's emission spectrum as a function of planetary longitude.
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CSI 2264: SIMULTANEOUS OPTICAL AND INFRARED LIGHT CURVES OF YOUNG DISK-BEARING STARS IN NGC 2264 WITH CoRoT and SPITZER—EVIDENCE FOR MULTIPLE ORIGINS OF VARIABILITY*
Ann Marie Cody,John R. Stauffer,Annie Baglin,Giuseppina Micela,Luisa Rebull,Ettore Flaccomio,Maria Morales-Calderon,Suzanne Aigrain,Jerome Bouvier,Lynne A. Hillenbrand,Robert A. Gutermuth,Inseok Song,Neal J. Turner,Silvia H. P. Alencar,Konstanze Zwintz,Peter Plavchan,John M. Carpenter,Krzysztof Findeisen,Sean Carey,Susan Terebey,Lee Hartmann,Nuria Calvet,Paula S. Teixeira,Frederick J. Vrba,Scott J. Wolk,Kevin R. Covey,Katja Poppenhaeger,Hans Moritz Günther,Jan Forbrich,Jan Forbrich,Barbara Whitney,Laura Affer,William Herbst,Joseph L. Hora,David Barrado,Jon Holtzman,Franck Marchis,Kenneth Wood,M. M. Guimarães,Jorge Lillo Box,Edward Gillen,Amy McQuillan,Catherine Espaillat,Lori Allen,Paola D'Alessio,Fabio Favata +45 more
TL;DR: The Coordinated Synoptic Investigation of NGC 2264 (CSI 2264) as discussed by the authors was a 30-day multi-wavelength photometric monitoring campaign on more than 1000 young star members using 16 telescopes.
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WASP-12b: the hottest transiting extrasolar planet yet discovered
Leslie Hebb,Andrew Collier-Cameron,B. Loeillet,Don Pollacco,Guillaume Hébrard,Rachel Street,François Bouchy,H. C. Stempels,C. Moutou,E. K. Simpson,Stéphane Udry,Yogesh C. Joshi,Richard G. West,I. Skillen,D. M. Wilson,Iain McDonald,Neale P. Gibson,Suzanne Aigrain,David R. Anderson,C. R. Benn,Damian J. Christian,B. Enoch,Carole A. Haswell,Coel Hellier,Keith Horne,Jonathan Irwin,T. A. Lister,Pierre F. L. Maxted,Michel Mayor,Andrew Norton,N. R. Parley,Frederic Pont,D. Queloz,Barry Smalley,Peter J. Wheatley +34 more
TL;DR: The planet has an equilibrium temperature of T eq = 2516 K caused by its very short period orbit around the hot, twelfth magnitude host star and has the largest radius of any transiting planet yet detected.
Journal ArticleDOI
Hubble Space Telescope Transmission Spectroscopy of the Exoplanet HD 189733b: High-altitude atmospheric haze in the optical and near-UV with STIS
David K. Sing,Frederic Pont,Suzanne Aigrain,D. Charbonneau,Jean-Michel Desert,Neale P. Gibson,R. L. Gilliland,Wolfgang Hayek,G. W. Henry,Heather Knutson,A. Lecavelier des Etangs,Tsevi Mazeh,A. Shporer +12 more
TL;DR: In this article, the authors used time series spectra obtained during two transit events to determine the wavelength dependance of the planetary radius and measure the exoplanet's atmospheric transmission spectrum for the first time over this wavelength range.