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91探花
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. Cal莽ada, Solar Dynamics Observatory

Prof Suzanne Aigrain

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics
  • Exoplanets and planetary physics

Sub department

  • Astrophysics

Research groups

  • Exoplanets and Stellar Physics
Suzanne.Aigrain@physics.ox.ac.uk
Telephone: 01865 (2)73339
Denys Wilkinson Building, room 762
  • About
  • Publications

Exoplanet atmospheres with EChO: spectral retrievals using EChOSim

(2014)

Authors:

Joanna K Barstow, Neil E Bowles, Suzanne Aigrain, Leigh N Fletcher, Patrick GJ Irwin, Ryan Varley, Enzo Pascale

CLOUDS ON THE HOT JUPITER HD189733b: CONSTRAINTS FROM THE REFLECTION SPECTRUM

The Astrophysical Journal American Astronomical Society 786:2 (2014) 154

Authors:

JK Barstow, S Aigrain, PGJ Irwin, T Hackler, LN Fletcher, JM Lee, NP Gibson

Exploring the diversity of Jupiter-class planets

Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences The Royal Society 372:2014 (2014) 20130064

Authors:

Leigh N Fletcher, Patrick GJ Irwin, Joanna K Barstow, Remco J de Kok, Jae-Min Lee, Suzanne Aigrain

CSI 2264: CHARACTERIZING ACCRETION-BURST DOMINATED LIGHT CURVES FOR YOUNG STARS IN NGC 2264**Based on data from the Spitzer and CoRoT missions, as well as the Canada鈥揊rance鈥揌awaii Telescope (CFHT) MegaCam CCD, and the European Southern Observatory Very Large Telescope, Paranal Chile, under program 088.C-0239. The CoRoT space mission was developed and is operated by the French space agency CNES, with participation of ESA's RSSD and Science Programmes, Austria, Belgium, Brazil, Germany, and Spain. MegaCam is a joint project of CFHT and CEA/DAPNIA, which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

The Astronomical Journal American Astronomical Society 147:4 (2014) 83

Authors:

John Stauffer, Ann Marie Cody, Annie Baglin, Silvia Alencar, Luisa Rebull, Lynne A Hillenbrand, Laura Venuti, Neal J Turner, John Carpenter, Peter Plavchan, Krzysztof Findeisen, Sean Carey, Susan Terebey, Mar铆a Morales-Calder贸n, Jerome Bouvier, Giusi Micela, Ettore Flaccomio, Inseok Song, Rob Gutermuth, Lee Hartmann, Nuria Calvet, Barbara Whitney, David Barrado, Frederick J Vrba, Kevin Covey, William Herbst, Gabor Furesz, Suzanne Aigrain, Fabio Favata

CSI 2264: SIMULTANEOUS OPTICAL AND INFRARED LIGHT CURVES OF YOUNG DISK-BEARING STARS IN NGC 2264 WITH CoRoT and SPITZER鈥擡VIDENCE FOR MULTIPLE ORIGINS OF VARIABILITY**Based on data from the Spitzer and CoRoT missions. The CoRoT space mission was developed and is operated by the French space agency CNES, with participation of ESA's RSSD and Science Programmes, Austria, Belgium, Brazil, Germany, and Spain.

The Astronomical Journal American Astronomical Society 147:4 (2014) 82

Authors:

Ann Marie Cody, John Stauffer, Annie Baglin, Giuseppina Micela, Luisa M Rebull, Ettore Flaccomio, Mar铆a Morales-Calder贸n, Suzanne Aigrain, J猫r么me Bouvier, Lynne A Hillenbrand, Robert Gutermuth, Inseok Song, Neal Turner, Silvia HP Alencar, Konstanze Zwintz, Peter Plavchan, John Carpenter, Krzysztof Findeisen, Sean Carey, Susan Terebey, Lee Hartmann, Nuria Calvet, Paula Teixeira, Frederick J Vrba, Scott Wolk, Kevin Covey, Katja Poppenhaeger, Hans Moritz G眉nther, Jan Forbrich, Barbara Whitney, Laura Affer, William Herbst, Joseph Hora, David Barrado, Jon Holtzman, Franck Marchis, Kenneth Wood, Marcelo Medeiros Guimar茫es, Jorge Lillo Box, Ed Gillen, Amy McQuillan, Catherine Espaillat, Lori Allen, Paola D'Alessio, Fabio Favata

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