Bibcode
Erikson, A.; Santerne, A.; Renner, S.; Barge, P.; Aigrain, S.; Alapini, A.; Almenara, J.-M.; Alonso, R.; Auvergne, M.; Baglin, A.; Benz, W.; Bonomo, A. S.; Bordé, P.; Bouchy, F.; Bruntt, H.; Cabrera, J.; Carone, L.; Carpano, S.; Csizmadia, Sz.; Deleuil, M.; Deeg, H. J.; Díaz, R. F.; Dvorak, R.; Ferraz-Mello, S.; Fridlund, M.; Gandolfi, D.; Gazzano, J.-C.; Gillon, M.; Guenther, E. W.; Guillot, T.; Hatzes, A.; Hébrard, G.; Jorda, L.; Lammer, H.; Léger, A.; Llebaria, A.; Mayor, M.; Mazeh, T.; Moutou, C.; Ollivier, M.; Ofir, A.; Pätzold, M.; Pepe, F.; Pont, F.; Queloz, D.; Rabus, M.; Rauer, H.; Régulo, C.; Rouan, D.; Samuel, B.; Schneider, J.; Shporer, A.; Tingley, B.; Udry, S.; Wuchterl, G.
Bibliographical reference
Astronomy and Astrophysics, Volume 539, id.A14
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3
2012
Journal
Citations
23
Refereed citations
20
Description
Context. The space mission CoRoT is 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 short run observed by CoRoT that targeted SRc01, towards the
Galactic center in the direction of Aquila, which lasted from April to
May 2007. Methods: Among the acquired data, we analyzed those for
1269 sources in the chromatic bands and 5705 in the monochromatic band.
Instrumental noise and the stellar variability were treated with several
detrending tools, to which several transit-search algorithms were
subsequently applied. Results: Fifty-one sources were classified
as planetary transit candidates and 26 were followed up with
ground-based observations. Until now, no planet has been detected in the
CoRoT data from the SRc01 field.
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. The CoRoT data are available
to the community from the CoRoT archive: http://idoc-corot.ias.u-psud.frBased
in part on observations made with the 1.93-m telescope at Observatoire
de Haute Provence (CNRS), France (SOPHIE Program 08A.PNP.MOUT).Based in
part on observations made with the ESO-3.60-m telescope at La Silla
Observatory (ESO), Chile (HARPS Program ESO - 081.C-0388) and with the
ESO-VLT telescope at Paranal Observatory (ESO), Chile (FLAMES Program
ESO - 081.C-0413).
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