[PDF] Top 20 Multiple star systems observed with CoRoT and Kepler
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Multiple star systems observed with CoRoT and Kepler
... strained. CoRoT was enlisted to help this issue through observations of the young open cluster NGC 2264, which is known to contain many young ...and CoRoT 223992193 has been studied in detail ... See full document
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Observations of binary stars with the differential speckle survey instrument. IV. Observations of Kepler, CoRoT, and Hipparcos stars from the Gemini North Telescope
... were observed to help determine the scale and orientation of the pixel axes with respect to celestial coordinates; (2) a number of targets observed below the diffraction limit at WIYN were observed ... See full document
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Derivation of the parameters of CoRoT planets
... as systems instead of separate objects, and a careful understanding of the observational and theoretical uncertainties (see in particular Sections 3 and ...(MOST, CoRoT, Kepler, CHEOPS, EChO, and ... See full document
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Probing the Deep End of the Milky Way with New Oscillating Kepler Giants
... from CoRoT [Con- vection, Rotation, and Transits 17] and Kepler have been combined to large spectroscopic surveys such as APOGEE [Apache Point Observatory Galactic Evolution Experi- ment 18] leading to ... See full document
5
Transiting exoplanets: From planet statistics to their physical nature
... The current space missions CoRoT and Kepler as well as future missions proposed in Europe (PLATO) and the U.S. (e.g. TESS, ASTRO) target the detection of small transit depths to fill the known planet mass ... See full document
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Transit timing observations from Kepler- III. Confirmation of four multiple planet systems by a Fourier-domain study of anticorrelated transit timing variations
... the star) assuming a cir- cular ...the Kepler bandpass (Claret ...these systems show visible TTVs, we display their light curves in Figs 1–4, where data are prepared (with TTVs corrected) as ... See full document
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Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data
... the observed light curve and uses this time-variable PSD estimate to realize a pre-whitening filter and whiten the light curve (Jenkins 2002; Jenkins et ...into multiple event statistics by folding them at ... See full document
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Architecture and dynamics of Kepler's candidate multiple transiting planet systems
... the observed distribution, a careful look at the histograms shown in Figure 11 reveals that the most common location for a pair of planets to reside is slightly exterior to the MMR (the planets are farther apart ... See full document
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Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models
... radius Kepler-30b should not be multiple Jupiter ...a multiple-planet system yet detected (but not quite rivaling the circumbinary planet Kepler-16(AB)b; Doyle et ...the observed signal ... See full document
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Planetary candidates observed by Kepler IV: Planet sample from Q1-Q8 (22 months)
... target star is not isolated but has contaminating flux in the aperture from other sources (Wielen ...48 Kepler long cadences ( ∼ 30 minutes in duration) and phase folded on the KOI ...flux observed ... See full document
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Self-gravitating disc candidates around massive young stars
... these systems, and their young ages, it is worth investigating their propensity to becoming ...those observed, with mid-plane dust temperatures comparable to measured temperatures from molecular line ... See full document
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Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data
... The modeling allows for the presence of a secondary eclipse (or occultation event) near phase = 0.5 as a means of identi- fying diluted or grazing eclipsing star systems. The Secondary Statistic (Column 8 ... See full document
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The orbit and mass of the third planet in the Kepler 56 system
... of multiple-planet systems have orbital angular momentum axes that align with the spin axis of their host star, Kepler-56 is an exception: its two transiting planets are coplanar yet ... See full document
7
Statistical properties of quasi periodic pulsations in white light flares observed with Kepler
... The Kepler mission made white-light observations of around 150,000 astrophysical targets between 2009 and ...makes Kepler suitable for studying QPPs with pe- riods greater than a few minutes, allowing for ... See full document
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Surface flux patterns on planets in circumbinary systems and potential for photosynthesis
... This spectral niche differentiation is seen on the Earth, across scales similar to that observed at different depths in the Earths oceans (Stomp et al., 2007; Raven, 2007). O’Malley-James et al. (2012) considered ... See full document
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Validation of 12 small Kepler transiting planets in the habitable zone
... in systems with five candidates each (KOI-0571.05 = Kepler- 186 f, ...= Kepler-296 f, and KOI-1422.05 = Kepler- 296 e) were the subject of recent studies by ... See full document
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A seismic and gravitationally bound double star observed by Kepler: implication for the presence of a convective core
... the Kepler data ...were observed by ...motion observed between 1850 and 2007 does not al- low one to derive a meaningful ...binary systems are clearly resolved such that the time series of ... See full document
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Revision of earth-sized Kepler planet candidate properties with high-resolution imaging by the Hubble space telescope
... GO-12893 observed 22 targets before 2014 May 1, six of which were found to be multiple star systems unresolved by ...perform multiple-star isochrone fi tting using the latest ... See full document
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On the relative sizes of planets within kepler multiple-candidate systems
... planetary systems takes a concerted ground-based observational and modeling effort to rule out false positives caused by blends ...the multiple-candidate systems provide additional information that ... See full document
12
CSI 2264 : accretion process in classical T Tauri stars in the young cluster NGC 2264
... As the star-disk system rotates, the observed Hα line of CTTSs varies in intensity and shape. This is expected to occur, even in a stable accretion regime, if the stellar magnetic and rotation axis are not ... See full document
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