Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-19T04:29:41.022Z Has data issue: false hasContentIssue false

CoRoT mission highlights

Published online by Cambridge University Press:  10 November 2011

Magali Deleuil
Affiliation:
Laboratoire d'Astrophysique de Marseille, 38 rue F. Joliot-Curie, 13388 Marseille Cedex 13, France email: [email protected], [email protected]
Pascal Bordé
Affiliation:
Institut d'Astrophysique Spatiale, Bât. 121, 91405 Orsay, France email: [email protected]
Claire Moutou
Affiliation:
Laboratoire d'Astrophysique de Marseille, 38 rue F. Joliot-Curie, 13388 Marseille Cedex 13, France email: [email protected], [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The CoRoT space telescope is detecting planets with the transit method for more than four years. Its tally includes hot jupiter planets with orbital periods up to 95 days but also the first Super-Earth, CoRoT-7b, whose density is similar to the Earth's one, as well as close-in brown dwarfs. We review the status of the CoRoT/Exoplanet program, including some elements of the multi step strategy of complementary observations. We then present some of the CoRoT exoplanetary systems and how they widen the range of properties of the close-in low mass population and contribute to our understanding of the properties of planets.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Aigrain, S., Collier-Cameron, A., Ollivier, M., et al. 2008, A&A, 488, L43Google Scholar
Alonso, R., Auvergne, M., Baglin, A., et al. 2008, A&A, 482, L21Google Scholar
Bonomo, A. S., Santerne, A., Alonso, R., et al. 2010, A&A, 520, 65Google Scholar
Bordé, P., Bouchy, F., Deleuil, M., et al. 2010, A&A, 520, 97Google Scholar
Bouchy, F., Moutou, C., & Queloz, D. 2009, Proc. IAU Symp. 253, 129Google Scholar
Bouchy, F., Deleuil, M., Guillot, T., et al. 2010, A&A, 525, 68Google Scholar
Cabrera, J., Fridlund, M., Ollivier, M., et al. 2009, A&A 506, 501Google Scholar
Deeg, H. J., Gillon, M., Shporer, A., et al. 2009, A&A, 506, 343Google Scholar
Deeg, H. J., Moutou, C., Erikson, A., et al. 2010, Nature, 464, 384CrossRefGoogle Scholar
Deleuil, M., Deeg, H. J., Alonso, R., et al. 2008, A&A, 491, 889Google Scholar
Gandolfi, D., Hébrard, G., Alonso, R., et al. 2010, A&A, 524, 55Google Scholar
Gazzano, J.-C., de Laverny, P., Deleuil, M., et al. 2011, (submitted to A&A)Google Scholar
Gillon, M., Lanotte, A. A., Barman, T., et al. 2010, A&A, 511, 3Google Scholar
Hatzes, A. P., Dvorak, R., Wuchterl, G., et al. 2010, A&A, 520, 93Google Scholar
Huber, K. F., Czesla, S., Wolter, U., & Schmitt, J. H. M. M. 2010, A&A, 514, A39Google Scholar
Huber, K. F., Czesla, S., Wolter, U., & Schmitt, J. H. M. M. 2009, A&A, 508, 901Google Scholar
Jackson, B., Greenberg, R., & Barnes, R. 2008, ApJ, 678, 1396CrossRefGoogle Scholar
Lanza, A. F., et al. 2009, A&A, 493, 193Google Scholar
Lanza, A. F., et al. 2009, A&A, 506, 255Google Scholar
Lanza, A. F., et al. 2011, A&A, 525, A14Google Scholar
Léger, A., et al. 2009, A&A, 506, 287Google Scholar
Ollivier, M., et al. 2011, A&A, to be submittedGoogle Scholar
Pont, F., Aigrain, S. & Zucker, S. 2011, MNRAS, 411, 1953CrossRefGoogle Scholar
Queloz, D., Bouchy, F., Moutou, C., et al. 2009, A&A, 506, 303Google Scholar
Rauer, H., Queloz, D., Csizmadia, Sz., et al. 2009, A&A, 506, 281Google Scholar
Silva-Valio, A., Lanza, A. F., Alonso, R., & Barge, P. 2010, A&A, 510, A25Google Scholar
Surace, C., Alonso, R., Barge, P. et al. 2008, SPIE, 7019, 111Google Scholar
Tingley, B., Endl, M., Gazzano, J.-C., et al. , 2011, A&A, 528, A97Google Scholar
Wolter, U., Schmitt, J. H. M. M., Huber, K. F., Czesla, S., Müller, H. M., Guenther, E. W., & Hatzes, A. P. 2009, A&A, 504, 561Google Scholar