Transit surveys

As a member of the science team for NASA’s Kepler mission, Ford and his research group contributed to the discovery and characterization of many interesting exoplanets. Now, most known exoplanets orbit stars with additional known planets. This presents new opportunities for using the relationships of planets in a system to understand the history of planet formation in these planetary systems.

Recently, our research group have focused on the characterization of exoplanet populations, combining rigorous statistical methods with a detailed understanding of the astronomical selection effects. Results are presented in a series of papers using “SysSim”, the Planetary Systems Simulator.

Confirming Planets using Transit Timing Variations

This animation shows the how planet transit times differ depending on whether the system contains one planet or multiple planets. (Credit: NASA Ames Research Center/Kepler Mission)

Publications

We present occurrence rates for rocky planets in the habitable zones (HZ) of main-sequence dwarf stars based on the Kepler DR25 planet …

We present robust planet occurrence rates for Kepler planet candidates around M stars for planet radii $Rp=0.5−4 R\oplus$ and orbital …

The angular momentum deficit (AMD) of a planetary system is a measure of its orbital excitation and a predictor of long–term …

We present robust planet occurrence rates for Kepler planet candidates around M stars for planet radii Rp=0.5−4 R⊕ and orbital …

We describe an efficient and automated technique for detecting circumbinary planets that transit their binary hosts in Kepler light …

Here we report the sizes and masses of three planets orbiting Kepler-138, a star much fainter and cooler than the Sun. We determine …

When an exoplanet transits across the face of its host star atoms and gases in its atmosphere absorb some of the starlight at specific …