J/A+A/482/L17ivo://CDS.VizieR/J/A+A/482/L17doi:10.26093/cds/vizier.34829017CDSBarge P.Baglin A.Auvergne M.Rauer H.Leger A.Schneider J.,Pont F.Aigrain S.Almenara J.-M.Alonso R.Barbieri M.Borde P.,Bouchy F.Deeg H.J.De la Reza R.Deleuil M.Dvorak R.Erikson A.,Fridlund M.Gillon M.Gondoin P.Guillot T.Hatzes A.Hebrard G.,Jorda L.Kabath P.Lammer H.Llebaria A.Loeillet B.Magain P.,Mazeh T.Moutou C.Ollivier M.Patzold M.Queloz D.Rouan D.,Shporer A.Wuchterl G.CDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frplanetary-nebulaephotometryradial-velocityThe pioneer space mission for photometric planet searches, CoRoT, steadily monitors about 12000 stars in each of its fields of view. Transit candidates can be detected early in the processing of the data and before the end of a run of observation. We report the detection of the first planet discovered by CoRoT and characterizing it with the help of follow-up observations.2008A&A...482L..17Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/482/L17CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/482/L17https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/482/L17http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/482/L17https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/482/L17https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/482/L17http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/482/L17GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefault