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Related papers: Noise properties of the CoRoT data: a planet-findi…

200 papers

Context. The CoRoT short runs give us the opportunity to observe a large variety of late-type stars through their solar-like oscillations. We report observations of the star HD175726 that lasted for 27 days during the first short run of the…

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

In this thesis we have analysed the time evolution of the photometric precision achieved by the space-based exoplanet-hunting mission CoRoT during its flight phase (2007-2012). This study of the noise level of CoRoT light curves has been…

Instrumentation and Methods for Astrophysics · Physics 2016-09-09 Ruben Asensio-Torres

Context. CoRoT light curves have an unprecedented photometric quality, having simultaneously a high signal-to-noise ratio, a long time span and a nearly continuous duty-cycle. Aims. We analyse the light-curves of four bright targets…

Solar and Stellar Astrophysics · Physics 2015-05-13 B. Mosser , F. Baudin , A. F. Lanza , J. C. Hulot , C. Catala , A. Baglin , M. Auvergne

The CoRoT space telescope observed nearly 160 000 light curves. Among the most outstanding is that of the young, active planet host star CoRoT-2A. In addition to deep planetary transits, the light curve of CoRoT-2A shows strong rotational…

Solar and Stellar Astrophysics · Physics 2016-05-25 Evangelos Nagel , Stefan Czesla , Jürgen H. M. M. Schmitt

As a planet eclipses its parent star, a dark spot on the surface of the star may be occulted, causing a detectable variation in the light curve. A total of 77 consecutive transit light curves of CoRoT-2 were observed with a high temporal…

Solar and Stellar Astrophysics · Physics 2015-05-14 Adriana Silva-Valio , A. F. Lanza , R. Alonso , P. Barge

When a planet occults a spotty area on a stellar surface, the flux increases and a characteristic feature in a light curve - a bump - is observed. Among the planets detected by the CoRoT-mission CoRoT-18 is especially interesting as it…

Earth and Planetary Astrophysics · Physics 2020-01-08 St. Raetz , A. M. Heras , P. Gondoin , M. Fernández , V. Casanova , T. O. B. Schmidt , G. Maciejewski

We present the preliminary results of the study of an interesting target in the first CoRoT exo-planet field (IRa1): CoRoT 102918586. Its light curve presents additional variability on the top of the eclipses, whose pattern suggests multi-…

Solar and Stellar Astrophysics · Physics 2010-04-12 C. Maceroni , D. Cardini , C. Damiani , D. Gandolfi , J. Debosscher , A. Hatzes , E. W. Guenther , C. Aerts

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…

CoRoT has allowed a quantitative leap for the solar-like-star seismology thanks to 5-month-long uninterrupted timeseries of high-precision photometric data. Kepler is also starting to deliver similar data. Now, several F and G main-sequence…

Solar and Stellar Astrophysics · Physics 2010-10-14 J. Ballot

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…

One of the objectives of the CoRoT mission is the search for transiting extrasolar planets using high-precision photometry, and the accurate characterization of their fundamental parameters. The CoRoT satellite consecutively observes…

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…

The lightcurve of CoRoT-2 shows substantial rotational modulation and deformations of the planet's transit profiles caused by starspots. We consistently model the entire lightcurve, including both rotational modulation and transits,…

Solar and Stellar Astrophysics · Physics 2015-05-18 K. F. Huber , S. Czesla , U. Wolter , J. H. M. M. Schmitt

The detection of pulsational frequencies in stellar photometry is required as input for asteroseismological modelling. The second short run (SRa02) of the CoRoT mission has provided photometric data of unprecedented quality and…

We analysed the chromatic data of the planetary transits observed with CoRoT to supply homogeneous time series in each of the CoRoT colours. In a first step, we cleaned the chromatic light curves from the contamination of nearby stars and…

Earth and Planetary Astrophysics · Physics 2015-06-11 F. Borsa , E. Poretti

We analyze the surface structure of the planet host star CoRoT-2a using a consistent model for both the `global' (i.e., rotationally modulated) lightcurve and the transit lightcurves, using data provided by the CoRoT mission. Selecting a…

Solar and Stellar Astrophysics · Physics 2015-05-14 K. F. Huber , S. Czesla , U. Wolter , J. H. M. M. Schmitt

Stellar activity is ubiquitous in late-type stars. The special geometry of eclipsing binary systems is particularly advantageous to study the stellar surfaces and activity. We present a detailed study of the 145 d CoRoT light curve of the…

Solar and Stellar Astrophysics · Physics 2019-04-12 S. Czesla , S. Terzenbach , R. Wichmann , J. H. M. M. Schmitt

CoRoT, the pioneer space-based transit search, steadily provides thousands of high-precision light curves with continuous time sampling over periods of up to 5 months. The transits of a planet perturbed by an additional object are not…

CoRoT-2, the second planet-hosting star discovered by the CoRoT satellite, is a young and active star. A total of 77 transits were observed for this system over a period of 135 days. Small modulations detected in the optical light curve of…

Solar and Stellar Astrophysics · Physics 2015-05-27 Adriana Silva-Valio , A. F. Lanza
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