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91̽»¨
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. Calçada, 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

ASTEP South: An Antarctic Search for Transiting ExoPlanets around the celestial South pole

(2009)

Authors:

Nicolas Crouzet, Tristan Guillot, Karim Agabi, Jean-Pierre Rivet, Erick Bondoux, Zalpha Challita, Yan Fanteï-Caujolle, François Fressin, Djamel Mékarnia, François-Xavier Schmider, Franck Valbousquet, Alain Blazit, Serge Bonhomme, Lyu Abe, Jean-Baptiste Daban, Carole Gouvret, Thomas Fruth, Heike Rauer, Anders Erikson, Mauro Barbieri, Suzanne Aigrain, Frédéric Pont

The secondary eclipse of the transiting exoplanet CoRoT-2b

Astronomy and Astrophysics 501:3 (2009)

Authors:

R Alonso, T Guillot, T Mazeh, S Aigrain, A Alapini, P Barge, A Hatzes, F Pont

Abstract:

We present a study of the light curve of the transiting exoplanet CoRoT-2b, aimed at detecting the secondary eclipse and measuring its depth. The data were obtained with the CoRoT satellite during its first run of more than 140 days. After filtering the low frequencies with a pre-whitening technique, we detect a 0.0060±0.0020% secondary eclipse centered on the orbital phase 0.494±0.006. Assuming a black-body emission of the planet, we estimate a surface brightness temperature of Tp,CoRoT = 1910+90-100 K. We provide the planet's equilibrium temperature and re-distribution factors as a function of the unknown amount of reflected light. The upper limit for the geometric albedo is 0.12. The detected secondary is the shallowest ever found. © 2009 ESO.

Transit timing analysis of CoRoT-1b

(2009)

Authors:

Sz Csizmadia, S Renner, P Barge, E Agol, S Aigrain, R Alonso, JM Almenara, AS Bonomo, P Borde, F Bouchy, J Cabrera, HJ Deeg, R De la Reza, M Deleuil, R Dvorak, A Erikson, EW Guenther, M Fridlund, P Gondoin, T Guillot, A Hatzes, L Jorda, H Lammer, C Lázaro, A Leger, A Llebaria, P Magain, C Moutou, M Ollivier, M Paetzold, D Queloz, H Rauer, D Rouan, J Schneider, G Wuchterl, D Gandolfi

Transiting exoplanets from the CoRoT space mission: VII. The "hot-Jupiter"-type planet CoRoT-5b

(2009)

Authors:

H Rauer, D Queloz, Sz Csizmadia, M Deleuil, R Alonso, S Aigrain, JM Almenara, M Auvergne, A Baglin, P Barge, P Borde, F Bouchy, H Bruntt, J Cabrera, L Carone, S Carpano, R De la Reza, HJ Deeg, R Dvorak, A Erikson, M Fridlund, D Gandolfi, M Gillon, T Guillot, E Guenther, A Hatzes, G Hebrard, P Kabath, L Jorda, H Lammer, A Leger, A Llebaria, P Magain, T Mazeh, C Moutou, M Ollivier, M Paetzold, F Pont, M Rabus, S Renner, D Rouan, A Shporer, B Samuel, J Schneider, AHMJ Triaud, G Wuchterl

The spin-orbit angle of the transiting hot jupiter CoRoT-1b

(2009)

Authors:

F Pont, M Endl, WD Cochran, SI Barnes, C Sneden, PJ MacQueen, C Moutou, S Aigrain, R Alonso, A Baglin, F Bouchy, M Deleuil, M Fridlund, G Hebrard, A Hatzes., T Mazeh, A Shporer

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