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Hunting for the lowest-mass exoplanets

Published online by Cambridge University Press:  10 November 2011

Francesco Pepe
Affiliation:
Observatoire Astronomique de l'Université de Genève, 51, ch. des Maillettes, CH-1290 Versoix, Switzerland, email: [email protected]
Michel Mayor
Affiliation:
Observatoire Astronomique de l'Université de Genève, 51, ch. des Maillettes, CH-1290 Versoix, Switzerland, email: [email protected]
Christophe Lovis
Affiliation:
Observatoire Astronomique de l'Université de Genève, 51, ch. des Maillettes, CH-1290 Versoix, Switzerland, email: [email protected]
Willy Benz
Affiliation:
Physikalisches Institut der Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland
François Bouchy
Affiliation:
Institut d'Astrophysique de Paris, 98bis, bd Arago, F-75014 Paris, France
Xavier Dumusque
Affiliation:
Observatoire Astronomique de l'Université de Genève, 51, ch. des Maillettes, CH-1290 Versoix, Switzerland, email: [email protected]
Didier Queloz
Affiliation:
Observatoire Astronomique de l'Université de Genève, 51, ch. des Maillettes, CH-1290 Versoix, Switzerland, email: [email protected]
Nuno C. Santos
Affiliation:
Centro de Astrofísica da Universidade do Porto (CAUP), Rua das Estrelas, P-4150-762 Porto, Portugal
Damien Ségransan
Affiliation:
Observatoire Astronomique de l'Université de Genève, 51, ch. des Maillettes, CH-1290 Versoix, Switzerland, email: [email protected]
Stéphane Udry
Affiliation:
Observatoire Astronomique de l'Université de Genève, 51, ch. des Maillettes, CH-1290 Versoix, Switzerland, email: [email protected]
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Abstract

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In order to understand general planet characteristics and constrain formation models it is necessary to scan over the widest possible parameter range of discovered systems. Due to detection biases, the domain of very-low mass planets had remained poorly explored. Only with improving measurement precision it has been possible to enter in the sub-Neptune mass range. The HARPS planet search program has been particularly efficient in detecting such ice giants and super earths. The present talk will summarize the obtained results and the characteristics of the low-mass population of exoplanets.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Andrae, R., Schulze-Hartung, T., & Melchior, P. 2010, arXiv:1012.3754v1Google Scholar
Correia, A., Udry, S., Mayor, M., et al. 2009, A&A, 496, 521Google Scholar
Correia, A. C. M., Couetdic, J., Laskar, J., et al. 2010, A&A, 511, A21Google Scholar
Dumusque, X., Udry, S., Lovis, C., Santos, N. C., & Monteiro, M. J. P. F. G. 2011a, A&A, 525, A140Google Scholar
Dumusque, X., Santos, N. C., Udry, S., Lovis, C., & Bonfils, X. 2011b, A&A, 527, A82Google Scholar
Fischer, D. & Valenti, J. 2005, ApJ, 622, 1102CrossRefGoogle Scholar
Gould, A., Dong, S., Gaudi, B. S., et al. 2010, ApJ, 720, 1073Google Scholar
Gregory, P. C. 2011, MNRAS in press (arXiv:1101.0800)Google Scholar
Latham, D. W., Stefanik, R. P., Mazeh, T., Mayor, M., & Burki, G. 1989, Nature, 339, 38CrossRefGoogle Scholar
Lovis, C., Mayor, M., Pepe, F., et al. 2006, Nature, 441, 305CrossRefGoogle Scholar
Lovis, C. & Pepe, F. 2007, A&A, 468, 1115Google Scholar
Lovis, C., Mayor, M., Bouchy, F., Pepe, F., Queloz, D., Udry, S., Benz, W., & Mordasini, C. 2009, Proc. IAU Symp., 253, 502Google Scholar
Lovis, C., Ségransan, D., Mayor, M., et al. 2011, A&A, 528, A112Google Scholar
Mayor, M., Pepe, F., Queloz, D., et al. 2003, The Messenger, 114, 20Google Scholar
Mayor, M. & Queloz, D. 1995, Nature, 378, 355CrossRefGoogle Scholar
Mayor, M. & Udry, S. 2008, Physica Scripta, 130, 014010Google Scholar
Mayor, M., Bonfils, X., Forveille, T., et al. 2009a, A&A, 507, 487Google Scholar
Mayor, M., Udry, S., Lovis, C., et al. 2009b, A&A, 493, 639Google Scholar
Mordasini, C., Alibert, Y., & Benz, W. 2009a, A&A, 501, 1139Google Scholar
Mordasini, C., Alibert, Y., Benz, W., & Naef, D. 2009b, A&A, 501, 1161Google Scholar
Pasquini, L., Cristiani, S., Garcia-Lopez, R., Haehnelt, M., & Mayor, M. 2010, The Messenger, 140, 20Google Scholar
Pepe, F., Correia, A. C. M., Mayor, M., et al. 2007, A&A, 462, 769Google Scholar
Pepe, F., Cristiani, S., Rebolo Lopez, R., et al. 2010, Proc. SPIE, 7735, 14Google Scholar
Pepe, F., et al. 2011, A&A, submittedGoogle Scholar
Rivera, E. J., Lissauer, J. J., Butler, R. P., et al. 2005, ApJ, 634, 625Google Scholar
Santos, N. C., Israelian, G., & Mayor, M. 2001, A&A, 373, 1019Google Scholar
Santos, N. C., Israelian, G., & Mayor, M. 2004, A&A, 415, 1153Google Scholar
Santos, N. C., Bouchy, F., Mayor, M., et al. 2004, A&A, 426, L19Google Scholar
Sousa, S. G., Santos, N. C., Mayor, M., et al. 2008, A&A, 487, 373Google Scholar
Udry, S., Mayor, M., Benz, W., et al. 2006, A&A, 447, 361Google Scholar
Udry, S., Bonfils, X., Delfosse, X., et al. 2007, A&A, 469, L43Google Scholar
Udry, S. & Mayor, M. 2008, ASP Conf. Ser., 398, 13Google Scholar
Vogt, S. S., Butler, R. P., Rivera, E. J., Haghighipour, N. H., Gregory, W. W., & Michael, H. 2010, ApJ, 723, 954CrossRefGoogle Scholar
Wilken, T., Lovis, C., Manescau, A., et al. 2010, MNRAS, 405, L16CrossRefGoogle Scholar