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dc.contributor.authorCarpano, S.en_GB
dc.contributor.authorCabrera, J.en_GB
dc.contributor.authorAlonso, R.en_GB
dc.contributor.authorBarge, P.en_GB
dc.contributor.authorAigrain, Suzanneen_GB
dc.contributor.authorAlmenara, J.-M.en_GB
dc.contributor.authorBordé, P.en_GB
dc.contributor.authorBouchy, F.en_GB
dc.contributor.authorCarone, L.en_GB
dc.contributor.authorDeeg, H. J.en_GB
dc.contributor.authorDe la Reza, R.en_GB
dc.contributor.authorDeleuil, M.en_GB
dc.contributor.authorDvorak, R.en_GB
dc.contributor.authorErikson, A.en_GB
dc.contributor.authorFressin, F.en_GB
dc.contributor.authorFridlund, M.en_GB
dc.contributor.authorGondoin, P.en_GB
dc.contributor.authorGuillot, T.en_GB
dc.contributor.authorHatzes, A.en_GB
dc.contributor.authorJorda, L.en_GB
dc.contributor.authorLammer, H.en_GB
dc.contributor.authorLéger, A.en_GB
dc.contributor.authorLlebaria, A.en_GB
dc.contributor.authorMagain, P.en_GB
dc.contributor.authorMoutou, C.en_GB
dc.contributor.authorOfir, A.en_GB
dc.contributor.authorOllivier, M.en_GB
dc.contributor.authorJanot-Pacheco, E.en_GB
dc.contributor.authorPätzold, M.en_GB
dc.contributor.authorPont, F.en_GB
dc.contributor.authorQueloz, D.en_GB
dc.contributor.authorRauer, H.en_GB
dc.contributor.authorRégulo, C.en_GB
dc.contributor.authorRenner, S.en_GB
dc.contributor.authorRouan, D.en_GB
dc.contributor.authorSamuel, B.en_GB
dc.contributor.authorSchneider, J.en_GB
dc.contributor.authorWuchterl, G.en_GB
dc.date.accessioned2009-11-26T15:26:20Zen_GB
dc.date.accessioned2011-01-25T11:54:28Zen_GB
dc.date.accessioned2013-03-20T13:20:57Z
dc.date.issued2009en_GB
dc.description.abstractContext. 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.en_GB
dc.identifier.citation506 (1), pp. 491-500en_GB
dc.identifier.doi10.1051/0004-6361/200911882en_GB
dc.identifier.urihttp://hdl.handle.net/10036/86949en_GB
dc.language.isoenen_GB
dc.publisherEDP Sciencesen_GB
dc.relation.urlhttp://dx.doi.org/10.1051/0004-6361/200911882en_GB
dc.subjectplanetary systemsen_GB
dc.subjectphotometric techniquesen_GB
dc.titlePlanetary transit candidates in Corot-IRa01 fielden_GB
dc.typeArticleen_GB
dc.date.available2009-11-26T15:26:20Zen_GB
dc.date.available2011-01-25T11:54:28Zen_GB
dc.date.available2013-03-20T13:20:57Z
dc.identifier.issn0004-6361en_GB
dc.identifier.issn1432-0746en_GB
dc.descriptionCopyright © The European Southern Observatory (ESO)en_GB
dc.identifier.journalAstronomy and Astrophysicsen_GB


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