III, T. N. Gautier
Latest
- Validation of Kepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-planet Systems
- Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets
- Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data
- On the Relative Sizes of Planets within Kepler Multiple-candidate Systems
- Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler
- Transit Timing Observations from Kepler. II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis
- Kepler-20: A Sun-like Star with Three Sub-Neptune Exoplanets and Two Earth-size Candidates
- Two Earth-sized planets orbiting Kepler-20
- Transiting circumbinary planets Kepler-34 b and Kepler-35 b
- Architecture and Dynamics of Kepler's Candidate Multiple Transiting Planet Systems
- Kepler-14b: A Massive Hot Jupiter Transiting an F Star in a Close Visual Binary
- Kepler-18b, c, and d: A System of Three Planets Confirmed by Transit Timing Variations, Light Curve Validation, Warm-Spitzer Photometry, and Radial Velocity Measurements
- The Distribution of Transit Durations for Kepler Planet Candidates and Implications for Their Orbital Eccentricities
- Transit Timing Observations from Kepler. I. Statistical Analysis of the First Four Months
- Characteristics of Planetary Candidates Observed by Kepler. II. Analysis of the First Four Months of Data
- A First Comparison of Kepler Planet Candidates in Single and Multiple Systems
- Kepler's First Rocky Planet: Kepler-10b
- A closely packed system of low-mass, low-density planets transiting Kepler-11
- Characteristics of Kepler Planetary Candidates Based on the First Data Set
- 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