Santos, N. C.[Centro de Astrofísica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal]
Moutou, C.[Laboratoire d'Astrophysique de Marseille, Traverse du Siphon, BP 8, Les Trois Lucs, 13376 Marseille Cedex 12, France]
Díaz, R. F.[Instituto de Astronomia y Física del Espacio (CONICET-UBA), Buenos Aires, Argentina]
Gieren, W.[Departamento de Fisica, Astronomy Group, Universidad de Concepción, Casilla 160-C, Concepción, Chile]
Gillon, Michaël[Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image >]
Hoyer, S.[Department of Astronomy, Universidad de Chile, Santiago, Chile]
Mayor, M.[Observatoire de Genève, 51 Chemin des Maillettes, 1290 Sauverny, Switzerland]
Mazeh, T.[School of Physics and Astronomy, R. and B. Sackler Faculty of Exact Sciences, Tel Aviv University, Tel Aviv, Israel]
Minniti, D.[Departmento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22, Chile]
Pietrzynski, G.[Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland; The OGLE Team; Departamento de Fisica, Astronomy Group, Universidad de Concepción, Casilla 160-C, Concepción, Chile]
Queloz, D.[Observatoire de Genève, 51 Chemin des Maillettes, 1290 Sauverny, Switzerland]
Ruiz, M. T.[Department of Astronomy, Universidad de Chile, Santiago, Chile]
Shporer, A.[School of Physics and Astronomy, R. and B. Sackler Faculty of Exact Sciences, Tel Aviv University, Tel Aviv, Israel]
Tamuz, O.[School of Physics and Astronomy, R. and B. Sackler Faculty of Exact Sciences, Tel Aviv University, Tel Aviv, Israel]
Udry, S.[Observatoire de Genève, 51 Chemin des Maillettes, 1290 Sauverny, Switzerland]
Zoccali, M.[Departmento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22, Chile]
Kubiak, M.[Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland; The OGLE Team]
Szymanski, M. K.[Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland]
Soszynski, I.[Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland]
Szewczyk, O.[Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland; The OGLE Team; Departamento de Fisica, Astronomy Group, Universidad de Concepción, Casilla 160-C, Concepción, Chile]
Ulaczyk, K.[Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland]
Wyrzykowski, L.[The OGLE Team; Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK]
[en] planetary systems ; stars: individual: OGLE-TR-211
[en] We present results of the photometric campaign for planetary and low-luminosity object transits conducted by the OGLE survey in the 2005 season (Campaign #5). About twenty of the most promising candidates discovered in these data were subsequently verified spectroscopically with the VLT/FLAMES spectrograph. One of the candidates, OGLE-TR-211, reveals clear changes of radial velocity with a small amplitude of 82 m/s, varying in phase with photometric transit ephemeris. Further analysis confirms the planetary nature of this system. Follow-up precise photometry of OGLE-TR-211 with VLT/FORS, together with radial velocity spectroscopy, supplemented with high-resolution, high S/N VLT/UVES spectra allowed us to derive parameters of the planet and host star. OGLE-TR-211b is a hot Jupiter orbiting an F7-8 spectral type dwarf star with a period of 3.68 days. The mass of the planet is equal to 1.03±0.20 M_Jup, while its radius 1.36[SUP]+0.18[/SUP][SUB]-0.09[/SUB] R_Jup. The radius is about 20% larger than the typical radius of hot Jupiters of similar mass. OGLE-TR-211b is, then, another example of inflated hot Jupiters - a small group of seven exoplanets with large radii and unusually low densities - objects that are a challenge to the current models of exoplanets. Based on observations made with the FORS1 camera and the FLAMES/UVES spectrograph at the VLT, ESO, Chile (program 07.C-0706, 076.C-0122, and 177.C-0666) and 1.3-m Warsaw Telescope at Las Campanas Observatory, Chile.