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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…

The mass of CoRoT-7b, the first transiting superearth exoplanet, is still a subject of debate. A wide range of masses have been reported in the literature ranging from as high as 8 M_Earth to as low as 2.3 M_Earth. Although most mass…

CoRoT-7 is an active star, whose orbiting planets and their masses have been under debate since their initial detection. In the previous studies, CoRoT-7 was found to have two planets, CoRoT-7b and CoRoT-7c with orbital periods of 0.85 and…

Earth and Planetary Astrophysics · Physics 2022-07-20 Ancy Anna John , Andrew Collier Cameron , Thomas G. Wilson

CoRoT-7b, the first super-Earth with measured radius discovered, has opened the new field of rocky exoplanets characterisation. To better understand this interesting system, new observations were taken with the CoRoT satellite. During this…

CoRoT-7 is an 11th magnitude K-star whose light curve shows transits with depth of 0.3 mmag and a period of 0.854 d, superimposed on variability at the 1% level, due to the modulation of evolving active regions with the star's 23 d rotation…

Earth and Planetary Astrophysics · Physics 2016-01-07 Frederic Pont , Suzanne Aigrain , Shay Zucker

Context. The CoRoT space mission routinely provides high-precision photometric measurements of thousands of stars that have been continuously observed for months. Aims. The discovery and characterization of the first very massive transiting…

Astrophysics · Physics 2009-11-13 M. Deleuil , H. J. Deeg , R. Alonso , F. Bouchy , D. Rouan

The detection and characterization of the first transiting super-Earth, CoRoT-7 b, has required an unprecedented effort in terms of telescope time and analysis. Although the star does display a radial velocity signal at the period of the…

Since the discovery of the transiting super-Earth CoRoT-7b, several investigations have yielded different results for the number and masses of planets present in the system, mainly owing to the star's high level of activity. We re-observed…

Aims. The CoRoT space mission continues to photometrically monitor about 12 000 stars in its field-of-view for a series of target fields to search for transiting extrasolar planets ever since 2007. Deep transit signals can be detected…

The up to 150 day uninterrupted high-precision photometry of about 100000 stars - provided so far by the exoplanet channel of the CoRoT space telescope - gave a new perspective on the planet population of our galactic neighbourhood. The…

Earth and Planetary Astrophysics · Physics 2015-05-14 R. Dvorak , J. Schneider , H. Lammer , P. Barge , G. Wuchterl , the CoRoT team

I report the results from a study of the transit times for CoRoT-1b, which was one of the first planets discovered by CoRoT. Analysis of the pipeline reduced CoRoT light curve yields a new determination of the physical and orbital…

Earth and Planetary Astrophysics · Physics 2015-05-13 Jacob L. Bean

Observations of transiting extrasolar planets are of key importance to our understanding of planets because their mass, radius, and mass density can be determined. The CoRoT space mission allows us to achieve a very high photometric…

High-energy irradiation of exoplanets has been identified to be a key influence on the stability of these planets' atmospheres. So far, irradiation-driven mass-loss has been observed only in two Hot Jupiters, and the observational data…

Solar and Stellar Astrophysics · Physics 2015-06-04 K. Poppenhaeger , S. Czesla , S. Schröter , S. Lalitha , V. Kashyap , J. H. M. M. Schmitt

We report the discovery of a massive and dense transiting planet CoRoT-27b on a 3.58 day orbit around a 4.2 Gyr-old G2 star. The planet candidate was identified from the CoRoT photometry, and was confirmed as a planet with ground-based…

The discovery of CoRoT-7b, a planet of radius 1.68 +/- 0.09 R_E, mass 4.8 +/- 0.8 M_E and orbital period of 0.854 days demonstrates that small planets can orbit extremely close to their star. We use knowledge of hot Jupiters, mass loss…

Earth and Planetary Astrophysics · Physics 2015-05-13 Diana Valencia , Masahiro Ikoma , Tristan Guillot , Nadine Nettelmann

Context. The pioneer space mission for photometric planet searches, CoRoT, steadily monitors about 12,000 stars in each of its fields of view; it is able to detect transit candidates early in the processing of the data and before the end of…

CONTEXT: The small radius and high density of CoRoT-7b implies that this transiting planet belongs to a differen t species than all transiting planets previously found. Current models suggest that this is the first transiting rocky planet…

Earth and Planetary Astrophysics · Physics 2015-05-20 E. W. Guenther , J. Cabrera , A. Erikson , M. Fridlund , H. Lammer , A. Mura , H. Rauer , J. Schneider , M. Tulej , Ph. von Paris , P. Wurz

Context. The CoRoT mission, a pioneer in exoplanet searches from space, has completed its first 150 days of continuous observations of ~12000 stars in the galactic plane. An analysis of the raw data identifies the most promising candidates…

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

This investigation uses the excellent HARPS radial velocity measurements of CoRoT-7 to re-determine the planet masses and to explore techniques able to determine mass and elements of planets discovered around active stars when the relative…

Earth and Planetary Astrophysics · Physics 2015-05-20 S. Ferraz-Mello , M. Tadeu dos Santos , C. Beauge , T. A. Michtchenko , A. Rodriguez
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