Bibcode
Carpano, S.; Cabrera, J.; Alonso, R.; Barge, P.; Aigrain, S.; Almenara, J.-M.; Bordé, P.; Bouchy, F.; Carone, L.; Deeg, H. J.; de La Reza, R.; Deleuil, M.; Dvorak, R.; Erikson, A.; Fressin, F.; Fridlund, M.; Gondoin, P.; Guillot, T.; Hatzes, A.; Jorda, L.; Lammer, H.; Léger, A.; Llebaria, A.; Magain, P.; Moutou, C.; Ofir, A.; Ollivier, M.; Janot-Pacheco, E.; Pätzold, M.; Pont, F.; Queloz, D.; Rauer, H.; Régulo, C.; Renner, S.; Rouan, D.; Samuel, B.; Schneider, J.; Wuchterl, G.
Bibliographical reference
Astronomy and Astrophysics, Volume 506, Issue 1, 2009, pp.491-500
Advertised on:
10
2009
Journal
Citations
40
Refereed citations
34
Description
Context: CoRoT is a pioneering space mission devoted to the analysis of
stellar variability and the photometric detection of extrasolar planets.
Aims: We present the list of planetary transit candidates detected
in the first field observed by CoRoT, IRa01, the initial run toward the
Galactic anticenter, which lasted for 60 days. Methods: We
analysed 3898 sources in the coloured bands and 5974 in the
monochromatic band. Instrumental noise and stellar variability were
taken into account using detrending tools before applying various
transit search algorithms. Results: Fifty sources were classified
as planetary transit candidates and the most reliable 40 detections were
declared targets for follow-up ground-based observations. Two of these
targets have so far been confirmed as planets, CoRoT-1b and CoRoT-4b,
for which a complete characterization and specific studies were
performed.
The CoRoT space mission, launched on December 27th 2006,
has been developed and is operated by CNES, with contributions from
Austria, Belgium, Brazil, ESA,
Germany, and Spain. Four
French laboratories associated with the CNRS (LESIA, LAM, IAS ,OMP)
collaborate with CNES on the satellite development.
First CoRoT data are available to the public from the CoRoT archive:
http://idoc-corot.ias.u-psud.fr.
Related projects
Helio and Astero-Seismology and Exoplanets Search
The principal objectives of this project are: 1) to study the structure and dynamics of the solar interior, 2) to extend this study to other stars, 3) to search for extrasolar planets using photometric methods (primarily by transits of their host stars) and their characterization (using radial velocity information) and 4) the study of the planetary
Savita
Mathur