Interests
- Planetary dynamics
- Extrasolar planetary systems
- Kuiper Belt Objects
- Astrostatistics
Latest
- The Occurrence of Rocky Habitable Zone Planets Around Solar-Like Stars from Kepler Data
- Architectures of Exoplanetary Systems: III. Eccentricity and Mutual Inclination Distributions of AMD–Stable Planetary Systems
- Architectures of Exoplanetary Systems. II: An Intrinsic Relation between Planetary System Occurrence and Spectral Type for Kepler's FGK Dwarfs
- Occurrence Rates of Planets Orbiting FGK Stars: Combining Kepler DR25, Gaia DR2, and Bayesian Inference
- Architectures of Exoplanetary Systems. I: A Clustered Forward Model for Exoplanetary Systems around Kepler's FGK Stars
- Improving the Accuracy of Planet Occurrence Rates from Kepler Using Approximate Bayesian Computation
- Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25
- A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets
- Kepler-1647b: The Largest and Longest-period Kepler Transiting Circumbinary Planet
- Transit Timing Observations from Kepler. IX. Catalog of the Full Long-cadence Data Set
- Architecture of Kepler's Multi-transiting Systems. II. New Investigations with Twice as Many Candidates
- Transit Timing Observations from Kepler. VIII. Catalog of Transit Timing Measurements of the First Twelve Quarters
- Kepler-68: Three Planets, One with a Density between that of Earth and Ice Giants
- A sub-Mercury-sized exoplanet
- 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
- The Neptune-sized Circumbinary Planet Kepler-38b
- Kepler-47: A Transiting Circumbinary Multiplanet System
- Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler
- Alignment of the stellar spin with the orbits of a three-planet system
- Almost All of Kepler's Multiple-planet Candidates Are Planets
- Kepler constraints on planets near hot Jupiters
- Transit Timing Observations from Kepler. II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis
- Transit Timing Observations from Kepler. IV. Confirmation of Four Multiple-planet Systems by Simple Physical Models
- 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-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
- The architecture of the hierarchical triple star KOI 928 from eclipse timing variations seen in Kepler photometry
- Kepler-16: A Transiting Circumbinary Planet
- 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
- KOI-126: A Triply Eclipsing Hierarchical Triple with Two Low-Mass Stars
- 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
- Five Kepler Target Stars That Show Multiple Transiting Exoplanet Candidates
- Kepler-9: A System of Multiple Planets Transiting a Sun-Like Star, Confirmed by Timing Variations