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Detection of small-size planetary candidates with CoRoT data

Published online by Cambridge University Press:  10 November 2011

Aldo S. Bonomo ,
Pierre-Yves Chabaud ,
Magali Deleuil ,
Claire Moutou  and
Pascal Bordé
Aldo S. Bonomo
Affiliation:
Laboratoire d'Astrophysique de Marseille, 38 rue Frédéric Joliot-Curie, 13388 Marseille Cedex 13, France email: [email protected]
Pierre-Yves Chabaud
Affiliation:
Laboratoire d'Astrophysique de Marseille, 38 rue Frédéric Joliot-Curie, 13388 Marseille Cedex 13, France email: [email protected]
Magali Deleuil
Affiliation:
Laboratoire d'Astrophysique de Marseille, 38 rue Frédéric Joliot-Curie, 13388 Marseille Cedex 13, France email: [email protected]
Claire Moutou
Affiliation:
Laboratoire d'Astrophysique de Marseille, 38 rue Frédéric Joliot-Curie, 13388 Marseille Cedex 13, France email: [email protected]
Pascal Bordé
Affiliation:
Institut d'Astrophysique Spatiale, centre universitaire d'Orsay Bât 120-121, 91405 ORSAY CEDEX
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Abstract

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With the discovery of CoRoT-7b, the first transiting super-Earth, the CoRoT space mission has shown the capability to detect short-period rocky planets around solar-like stars. By performing a blind test with real CoRoT light curves, we want to establish the detection threshold of small-size planets in CoRoT data. We investigate the main obstacles to the detection of transiting super-Earths in CoRoT data, notably the presence of short-time scale variability and hot pixels.

Keywords

methods: data analysistechniques: photometricstars: late-type
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S276: The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution , October 2010 , pp. 523 - 524
Copyright
Copyright © International Astronomical Union 2011

References

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