[PDF] Top 20 Almost all of Kepler's multiple-planet candidates are planets
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Almost all of Kepler's multiple-planet candidates are planets
... by planets from FPs produced by known astrophysical ...a planet transiting the target star and a vast array of possible astrophysical FPs involving binary stars and larger planets transiting fainter ... See full document
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Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems
... of all of the validated planets in systems with a newly validated planet with S < ...and planet candidates to a uniform ...Verified planets are shown in black while ... See full document
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A catalog of Kepler habitable zone exoplanet candidates
... of Kepler candidates that lie in the HZ of their host ...of candidates allow the reader to adopt the criteria that are most useful for a particular follow-up ...giant planets in the optimistic ... See full document
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The orbit and mass of the third planet in the Kepler 56 system
... . Kepler- 56 d ’ s minimum mass could be commensurate with that of a giant planet or a brown dwarf ( for inclinations below 30 °) ...inner planets ’ orbits, as well as for the misalignment of ... See full document
7
Validation of 12 small Kepler transiting planets in the habitable zone
... recently Kepler-186 f (1.11 ± 0.14 R ⊕ ; Quintana et al. 2014). All of these were “validated” statistically using techniques such as BLENDER (Torres et ...most candidates in multis are very likely to ... See full document
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A 1.9 Earth Radius Rocky Planet and the Discovery of a Non-Transiting Planet in the Kepler-20 System
... the Kepler-20 planets based on analyses of the first two years of Kepler ...Although Kepler-20 was observed at short cadence (integration time per data point of ...58.8 s) beginning in ... See full document
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Modeling Kepler transit light curves as false positives: rejection of blend scenarios for Kepler-9, and validation of Kepler-9 d, a super-earth-size planet in a multiple system
... of Kepler, as well as the very high astrometric precision achieved in determining the centroids of the stars (see also Steffen et ...smallest planets; (3) checking for ellipsoidal variations, which could be ... See full document
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197 candidates and 104 validated planets in K2's first five fields
... As part of our false positive analysis ( described in Section 6 ) , we use our high-resolution Keck / HIRES spectra to search for additional spectral lines in the stellar spectra. This method is sensitive to secondary ... See full document
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Stability of exomoons around the Kepler transiting circumbinary planets
... the Kepler mission are transiting circumbinary planets (CBPs), ...i.e., planets in nearly-coplanar orbits around a stellar binary (and nearly copla- nar with the plane of the sky), temporarily ... See full document
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Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets
... the planets orbiting 22 Kepler stars. There are 49 planet candidates around these stars, including 42 detected through transits and 7 revealed by precise Doppler measurements of the host ... See full document
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Kepler's first rocky planet: Kepler-10b
... June, Kepler released a catalog of 306 stars with planet-like transit signatures (Borucki et ...transiting planets could plausibly more than double from this pool of ...from ... See full document
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Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models
... other Kepler confirmations so far, which have mostly relied on ground- based (and Spitzer Space Telescope) follow-up to confirm the planetary nature of the transiting ...candidate planets have been found, ... See full document
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The kepler-19 system: a transiting 2.2 R ⊕ planet and a second planet detected via transit timing variations
... Transiting planets are also of interest as they present an opportunity to identify yet more planets in the system by the method of transit timing variations ...for planets by TTVs has been a major ... See full document
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Seismology of Giant Planets: General Overview and Results from the Kepler K2 Observations of Neptune
... Regarding Saturn, Marley & Porco (1993) [29] en- visionned that “the rings of Saturn may act as a seis- mograph, recording gravitational perturbations associated with acoustic oscillations modes of the ... See full document
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Catching a Planet: A Tidal Capture Origin for the Oxomoon Candidate Kepler 1625b I
... of planets in such an environment is to be expected, in particular when the residual gas causes a drag force on the ...the planet mass ( Dürmann & Kley 2015 ) ...two planets have to acquire ... See full document
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Kepler 21b : a rocky planet around a V = 8 25 mag star
... brightest planet host star discovered by the Kepler ...m s −1 ...of Kepler-21 is similar to the bright targets to be observed by TESS and many of those targets will most likely have ... See full document
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Discovery and atmospheric characterization of giant planet Kepler-12b: An inflated radius outlier
... To model the planet’s atmosphere we use a one-dimensional plane-parallel atmosphere code that has been widely used for solar system planets, exoplanets, and brown dwarfs over the past two decades. The optical and ... See full document
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High-resolution multi-band imaging for validation and characterization of small Kepler planets
... candidate planets identi fi ed by the NASA Kepler ...into Kepler light curves, affecting estimated planet properties, and are important for an understanding of planets in multiple ... See full document
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Planet occurrence within 0.25AU of solar-type stars from Kepler
... of planets in the mass/orbital–period plane reveals important clues about planet formation and ...epochal Kepler results for transiting planet candidates from Borucki et ...the ... See full document
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The mass of Kepler 93b and the composition of terrestrial planets
... 58.5 s) beginning in Quarter 2 and extending until the end of the ...the Kepler-93 observations, the planet was detected in the first four months of Kepler data (Borucki et ...of ... See full document
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