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
Photometry of very bright stars with Kepler and K2 smear data
Benjamin J. S. Pope,Timothy R. White,Daniel Huber,Daniel Huber,Daniel Huber,Simon J. Murphy,Simon J. Murphy,Timothy R. Bedding,Timothy R. Bedding,Douglas A. Caldwell,Douglas A. Caldwell,Aleksa Sarai,Suzanne Aigrain,Thomas Barclay +13 more
TL;DR: In this article, the authors show that engineering data acquired for photometric calibration, consisting of collateral'smear' measuremen, can be used to reconstruct light curves for bright targets not otherwise observable with Kepler/K2.
Journal ArticleDOI
HII 2407: An Eclipsing Binary Revealed By K2 Observations of the Pleiades
Trevor J. David,John R. Stauffer,Lynne A. Hillenbrand,Ann Marie Cody,Kyle E. Conroy,Keivan G. Stassun,Keivan G. Stassun,Benjamin J. S. Pope,Suzanne Aigrain,Edward Gillen,Andrew Collier Cameron,David Barrado,L. M. Rebull,Howard Isaacson,Geoffrey W. Marcy,Celia Zhang,Reed Riddle,Carl Ziegler,Nicholas M. Law,Christoph Baranec +19 more
TL;DR: In this article, the National Science Foundation Graduate Research Fellowship under grant No. DGE1144469 was used to support the work of T.C.J.B., who was partially supported by an appointment to the NASA Postdoctoral Program at the Ames Research Center administered by Oak Ridge Associated Universities through a contract with NASA.
Journal ArticleDOI
How does thermal scattering shape the infrared spectra of cloudy exoplanets? A theoretical framework and consequences for atmospheric retrievals in the JWST era
Jake Taylor,Vivien Parmentier,Michael R. Line,Elspeth K. H. Lee,Patrick G. J. Irwin,Suzanne Aigrain +5 more
TL;DR: In this paper, the effects of thermal scattering on the emission spectra of hot Jupiter atmospheres were explored by modelling a suite of hot JWST atmospheres with varying cloud single-scattering albedos (SSAs) and temperature profiles.
Journal ArticleDOI
Transiting exoplanets from the CoRoT space mission. XXI. CoRoT-19b: a low density planet orbiting an old inactive F9V-star
E. W. Guenther,Rodrigo F. Díaz,Rodrigo F. Díaz,J. C. Gazzano,Tsevi Mazeh,Daniel Rouan,Neale P. Gibson,Sz. Csizmadia,Suzanne Aigrain,Roi Alonso,J. M. Almenara,Michel Auvergne,Annie Baglin,Pierre Barge,Aldo S. Bonomo,Pascal Bordé,François Bouchy,François Bouchy,Hans Bruntt,Juan Cabrera,Ludmila Carone,S. Carpano,C. Cavarroc,Hans J. Deeg,Hans J. Deeg,Magali Deleuil,Stefan Dreizler,Rudolf Dvorak,Anders Erikson,Sylvio Ferraz-Mello,M. Fridlund,Davide Gandolfi,Michaël Gillon,Tristan Guillot,Artie P. Hatzes,M. Havel,Guillaume Hébrard,Guillaume Hébrard,Emmanuel Jehin,Laurent Jorda,Helmut Lammer,A. Léger,C. Moutou,Lisa Nortmann,M. Ollivier,Aviv Ofir,T. Pasternacki,Martin Paetzold,Hannu Parviainen,Hannu Parviainen,Didier Queloz,Heike Rauer,Heike Rauer,B. Samuel,Alexandre Santerne,Jean Schneider,Lev Tal-Or,B. Tingley,B. Tingley,J. Weingrill,G. Wuchterl +60 more
TL;DR: In this paper, a gas-giant exoplanet CoRoT-19b was discovered, which is an example of a giant planet of almost the same mass as Jupiter but a 30% larger radius.
Journal ArticleDOI
Transiting exoplanets from the CoRoT space mission - XXVII. CoRoT-28b, a planet orbiting an evolved star, and CoRoT-29b, a planet showing an asymmetric transit
Juan Cabrera,Sz. Csizmadia,G. Montagnier,Malcolm Fridlund,Malcolm Fridlund,Malcolm Fridlund,M. Ammler-von Eiff,S. Chaintreuil,Cilia Damiani,Magali Deleuil,Sylvio Ferraz-Mello,A. Ferrigno,Davide Gandolfi,Tristan Guillot,E. W. Guenther,Artie P. Hatzes,Guillaume Hébrard,P. Klagyivik,P. Klagyivik,Hannu Parviainen,T. Pasternacki,Martin Pätzold,Daniel Sebastian,M. Tadeu dos Santos,G. Wuchterl,Suzanne Aigrain,Roi Alonso,Roi Alonso,J. M. Almenara,James D. Armstrong,James D. Armstrong,Michel Auvergne,Annie Baglin,Pierre Barge,S. C. C. Barros,Aldo S. Bonomo,Pascal Bordé,François Bouchy,S. Carpano,C. Chaffey,Hans J. Deeg,Hans J. Deeg,Rodrigo F. Díaz,Rudolf Dvorak,Anders Erikson,S. Grziwa,Judith Korth,Helmut Lammer,C. Lindsay,Tsevi Mazeh,C. Moutou,Aviv Ofir,Marc Ollivier,Enric Palle,Enric Palle,Heike Rauer,Heike Rauer,Daniel Rouan,B. Samuel,Alexandre Santerne,J. Schneider +60 more
TL;DR: In this article, the authors used the transit light curve to characterize the planetary parameters relative to the stellar parameters, which allowed them to further investigate the formation and evolution of the planetary systems and the main properties of the host stars.