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Related papers: XX. CoRoT-20b: A very high density, high eccentric…

200 papers

We report the discovery of the super-Earth K2-265 b detected with K2 photometry. The planet orbits a bright (V_mag = 11.1) star of spectral type G8V with a period of 2.37 days. We obtained high-precision follow-up radial velocity…

We report the discovery and confirmation of Kepler-7b, a transiting planet with unusually low density. The mass is less than half that of Jupiter, Mp = 0.43 Mj, but the radius is fifty percent larger, Rp = 1.48 Rj. The resulting density,…

We report the discovery of the low-density, transiting giant planet WASP-31b. The planet is 0.48 Jupiter masses and 1.55 Jupiter radii. It is in a 3.4-day orbit around a metal-poor, late-F-type, V = 11.7 dwarf star, which is a member of a…

We report the discovery of very shallow (DF/F = 3.4 10-4), periodic dips in the light curve of an active V = 11.7 G9V star observed by the CoRoT satellite, which we interpret as due to the presence of a transiting companion. We describe the…

CoRoT, the first space-based transit search, provides ultra-high precision light curves with continuous time-sampling over periods, of up to 5 months. This allows the detection of transiting planets with relatively long periods, and the…

We report the discovery of HAT-P-30b, a transiting exoplanet orbiting the V=10.419 dwarf star GSC 0208-00722. The planet has a period P=2.810595+/-0.000005 d, transit epoch Tc = 2455456.46561+/-0.00037 (BJD), and transit duration…

We report the discovery of an additional substellar companion in the CoRoT-20 system based on six years of HARPS and SOPHIE radial velocity follow-up. CoRoT-20 c has a minimum mass of 17 $\pm$ 1 $M_{Jup}$ and it orbits the host star in…

We report the discovery of a planet transiting a moderately faint (V=12.3 mag) late F star, with an orbital period of 3.92289 +/- 0.00004 days. From the transit light curve and radial velocity measurements we determine that the radius of…

We report the discovery of a new transiting planet in the Southern Hemisphere. It has been found by the WASP-south transit survey and confirmed photometrically and spectroscopically by the 1.2m Swiss Euler telescope, LCOGT 2m Faulkes South…

Accurate parameters of the host stars of exoplanets are important for the interpretation of the new planet systems that continue to emerge. The CoRoT satellite recently discovered a transiting rocky planet with a density similar to the…

Solar and Stellar Astrophysics · Physics 2015-05-19 H. Bruntt , M. Deleuil , M. Fridlund , R. Alonso , F. Bouchy , A. Hatzes , M. Mayor , C. Moutou , D. Queloz

We report the discovery of a massive (Mp = 9.04+/-0.50 MJup) planet transiting the bright (V = 8.7) F8 star HD 147506, with an orbital period of 5.63341+/-0.00013 days and an eccentricity of e = 0.520+/-0.010. From the transit light curve…

We report the discovery of HAT-P-14b, a fairly massive transiting extrasolar planet orbiting the moderately bright star GSC 3086-00152 (V = 9.98), with a period of P = 4.627669 +/- 0.000005 days. The transit is close to grazing (impact…

We describe the discovery of HAT-P-4b, a low-density extrasolar planet transiting BD+36 2593, a V = 11.2 mag slightly evolved metal-rich late F star. The planet's orbital period is 3.056536+/-0.000057 d with a mid-transit epoch of…

We present the study of the CoRoT transiting planet candidate 101186644, also named LRc01_E1_4780. Analysis of the CoRoT lightcurve and the HARPS spectroscopic follow-up observations of this faint (m_V = 16) candidate revealed an eclipsing…

Earth and Planetary Astrophysics · Physics 2015-06-15 L. Tal-Or , T. Mazeh , R. Alonso , F. Bouchy , J. Cabrera , H. J. Deeg , M. Deleuil , S. Faigler , M. Fridlund , G. Hebrard , C. Moutou , A. Santerne , B. Tingley

Statistical analyses from exoplanet surveys around low-mass stars indicate that super-Earth and Neptune-mass planets are more frequent than gas giants around such stars, in agreement with core accretion theory of planet formation. Using…

Earth and Planetary Astrophysics · Physics 2019-10-16 J. C. Morales , A. J. Mustill , I. Ribas , M. B. Davies , A. Reiners , F. F. Bauer , D. Kossakowski , E. Herrero , E. Rodríguez , M. J. López-González , C. Rodríguez-López , V. J. S. Béjar , L. González-Cuesta , R. Luque , E. Pallé , M. Perger , D. Baroch , A. Johansen , H. Klahr , C. Mordasini , G. Anglada-Escudé , J. A. Caballero , M. Cortés-Contreras , S. Dreizler , M. Lafarga , E. Nagel , V. M. Passegger , S. Reffert , A. Rosich , A. Schweitzer , L. Tal-Or , T. Trifonov , M. Zechmeister , A. Quirrenbach , P. J. Amado , E. W. Guenther , H. -J. Hagen , T. Henning , S. V. Jeffers , A. Kaminski , M. Kürster , D. Montes , W. Seifert , F. J. Abellán , M. Abril , J. Aceituno , F. J. Aceituno , F. J. Alonso-Floriano , M. Ammler-von Eiff , R. Antona , B. Arroyo-Torres , M. Azzaro , D. Barrado , S. Becerril-Jarque , D. Benítez , Z. M. Berdiñas , G. Bergond , M. Brinkmöller , C. del Burgo , R. Burn , R. Calvo-Ortega , J. Cano , M. C. Cárdenas , C. Cardona Guillén , J. Carro , E. Casal , V. Casanova , N. Casasayas-Barris , P. Chaturvedi , C. Cifuentes , A. Claret , J. Colomé , S. Czesla , E. Díez-Alonso , R. Dorda , A. Emsenhuber , M. Fernández , A. Fernández-Martín , I. M. Ferro , B. Fuhrmeister , D. Galadí-Enríquez , I. Gallardo Cava , M. L. García Vargas , A. Garcia-Piquer , L. Gesa , E. González-Álvarez , J. I. González Hernández , R. González-Peinado , J. Guàrdia , A. Guijarro , E. de Guindos , A. P. Hatzes , P. H. Hauschildt , R. P. Hedrosa , I. Hermelo , R. Hernández Arabi , F. Hernández Otero , D. Hintz , G. Holgado , A. Huber , P. Huke , E. N. Johnson , E. de Juan , M. Kehr , J. Kemmer , M. Kim , J. Klüter , A. Klutsch , F. Labarga , N. Labiche , S. Lalitha , M. Lampón , L. M. Lara , R. Launhardt , F. J. Lázaro , J. -L. Lizon , M. Llamas , N. Lodieu , M. López del Fresno , J. F. López Salas , J. López-Santiago , H. Magán Madinabeitia , U. Mall , L. Mancini , H. Mandel , E. Marfil , J. A. Marín Molina , E. L. Martín , P. Martín-Fernández , S. Martín-Ruiz , H. Martínez-Rodríguez , C. J. Marvin , E. Mirabet , A. Moya , V. Naranjo , R. P. Nelson , L. Nortmann , G. Nowak , A. Ofir , J. Pascual , A. Pavlov , S. Pedraz , D. Pérez Medialdea , A. Pérez-Calpena , M. A. C. Perryman , O. Rabaza , A. Ramón Ballesta , R. Rebolo , P. Redondo , H. -W. Rix , F. Rodler , A. Rodríguez Trinidad , S. Sabotta , S. Sadegi , M. Salz , E. Sánchez-Blanco , M. A. Sánchez Carrasco , A. Sánchez-López , J. Sanz-Forcada , P. Sarkis , L. F. Sarmiento , S. Schäfer , M. Schlecker , J. H. M. M. Schmitt , P. Schöfer , E. Solano , A. Sota , O. Stahl , S. Stock , T. Stuber , J. Stürmer , J. C. Suárez , H. M. Tabernero , S. M. Tulloch , G. Veredas , J. I. Vico-Linares , F. Vilardell , K. Wagner , J. Winkler , V. Wolthoff , F. Yan , M. R. Zapatero Osorio

CoRoT-7b, the first transiting ``superearth'' exoplanet, has a radius of 1.7 R_Earth and a mass of 4.8 M_Earth. Ground-based radial velocity measurements also detected an additional companion with a period of 3.7 days (CoRoT-7c) and a mass…

Solar and Stellar Astrophysics · Physics 2015-05-19 A. P. Hatzes , R. Dvorak , G. Wuchterl , P. Guterman , M. Hartmann , M. Fridlund , D. Gandolfi , E. Guenther , M. Paetzold

We report the discovery of K2-287b, a Saturn mass planet orbiting a G-dwarf with a period of $P \approx 15$ days. First uncovered as a candidate using K2 campaign 15 data, follow-up photometry and spectroscopy were used to determine a mass…

Despite the severe bias of the transit method of exoplanet discovery toward short orbital periods, a modest sample of transiting exoplanets with orbital periods greater than 100 days is known. Long-term radial velocity (RV) surveys are…