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This article summarizes a workshop held on March, 2014, on the potential ofthe James Webb Space Telescope (JWST) to revolutionize our knowledge of thephysical properties of exoplanets through transit observations. JWST's uniquecombination of high sensitivity and broad wavelength coverage will enable theaccurate measurement of transits with high signal-to-noise. Most importantly,JWST spectroscopy will investigate planetary atmospheres to determine atomicand molecular compositions, to probe vertical and horizontal structure, and tofollow dynamical evolution, i.e. exoplanet weather. JWST will sample a diversepopulation of planets of varying masses and densities in a wide variety ofenvironments characterized by a range of host star masses and metallicities,orbital semi-major axes and eccentricities. A broad program of exoplanetscience could use a substantial fraction of the overall JWST mission.

Observations of Transiting Exoplanets with the James Webb Space  Telescope (JWST), Publications of the Astronomical Society of the Pacific  (PASP), December 2014