T. M. Brown
Latest
- Low False Positive Rate of Kepler Candidates Estimated From A Combination Of Spitzer And Follow-Up Observations
- 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
- Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler
- Discovery and Atmospheric Characterization of Giant Planet Kepler-12b: An Inflated Radius Outlier
- 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 Atmospheres of the Hot-Jupiters Kepler-5b and Kepler-6b Observed during Occultations with Warm-Spitzer and Kepler
- The Hot-Jupiter Kepler-17b: Discovery, Obliquity from Stroboscopic Starspots, and Atmospheric Characterization
- 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
- 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
- Kepler-9: A System of Multiple Planets Transiting a Sun-Like Star, Confirmed by Timing Variations