Observations of Transiting Exoplanets with the James Webb Space Telescope (JWST)

@article{Beichman2014ObservationsOT,
  title={Observations of Transiting Exoplanets with the James Webb Space Telescope (JWST)},
  author={Charles A. Beichman and Bjoern Benneke and Heather A. Knutson and Roger M. Smith and Courtney D. Dressing and David W. Latham and Drake L. Deming and Jonathan I. Lunine and Pierre Olivier Lagage and Alessandro Sozzetti and David K. Sing and Eliza M.-R. Kempton and George R. Ricker and Jacob L. Bean and Laura Kreidberg and Jeroen Bouwman and Ian J. M. Crossfield and Jessie L. Christiansen and David R. Ciardi and Jonathan J. Fortney and Loic Albert and Ren{\'e} Doyon and Marcia J. Rieke and George H. Rieke and Mark C. Clampin and Matthew Greenhouse and Paul Goudfrooij and Dean C. Hines and Tony Keyes and Janice C. Lee and Peter R. McCullough and Massimo Robberto and J. Stansberry and Jeff A. Valenti and Pieter D. Deroo and Avi M. Mandell and Michael E. Ressler and Avi Shporer and Mark R. Swain and Gautam Vasisht and Sean J. Carey and Jessica E. Krick and Stephan M. Birkmann and Pierre Ferruit and Giovanna Giardino and Tom Greene and Steve B. Howell},
  journal={Publications of the Astronomical Society of the Pacific},
  year={2014},
  volume={126},
  pages={1134 - 1173}
}
This article summarizes a workshop held on March, 2014, on the potential of the James Webb Space Telescope (JWST) to revolutionize our knowledge of the physical properties of exoplanets through transit observations. JWST’s unique combination of high sensitivity and broad wavelength coverage will enable the accurate measurement of transits with high signal-to-noise ratio (S/N). Most importantly, JWST spectroscopy will investigate planetary atmospheres to determine atomic and molecular… 

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References

SHOWING 1-10 OF 87 REFERENCES

The K2 Mission: Characterization and Early Results

The K2 mission will make use of the Kepler spacecraft and its assets to expand upon Kepler’s groundbreaking discoveries in the fields of exoplanets and astrophysics through new and exciting

A super-Earth transiting a nearby low-mass star

Observations of the transiting planet GJ’1214b are reported, finding that the planetary mass and radius are consistent with a composition of primarily water enshrouded by a hydrogen–helium envelope that is only 0.05% of the mass of the planet.

Transiting Exoplanet Survey Satellite

Abstract. The Transiting Exoplanet Survey Satellite (TESS) will search for planets transiting bright and nearby stars. TESS has been selected by NASA for launch in 2017 as an Astrophysics Explorer

TWO NEARBY SUB-EARTH-SIZED EXOPLANET CANDIDATES IN THE GJ 436 SYSTEM

We report the detection of UCF-1.01, a strong exoplanet candidate with a radius 0.66 ± 0.04 times that of Earth (R⊕). This sub-Earth-sized planet transits the nearby M-dwarf star GJ 436 with a period

Discovery and Characterization of Transiting Super Earths Using an All-Sky Transit Survey and Follow-up by the James Webb Space Telescope

Doppler and transit surveys are finding extrasolar planets of ever smaller mass and radius, and are now sampling the domain of super Earths (1–3R⊕). Recent results from the Doppler surveys suggest

Precision Near-Infrared Photometry for Exoplanet Transit Observations. I. Ensemble Spot Photometry for an All-Sky Survey

Near-IR observations are important for the detection and characterization of exoplanets using the transit technique, either in surveys of large numbers of stars or for follow-up spectroscopic

Resolving the Surfaces of Extrasolar Planets with Secondary Eclipse Light Curves

We present a method that employs the secondary eclipse light curves of transiting extrasolar planets to probe the spatial variation of their thermal emission. This technique permits an observer to

Transiting Exoplanet Survey Satellite (TESS)

The Transiting Exoplanet Survey Satellite (TESS ) will search for planets transiting bright and nearby stars. TESS has been selected by NASA for launch in 2017 as an Astrophysics Explorer mission.

CHEOPS: A transit photometry mission for ESA's small mission programme

Ground based radial velocity (RV) searches continue to discover exoplanets below Neptune mass down to Earth mass. Furthermore, ground based transit searches now reach milli-mag photometric precision

The habitable zone planet finder: a proposed high-resolution NIR spectrograph for the Hobby Eberly Telescope to discover low-mass exoplanets around M dwarfs

The Habitable Zone Planet Finder (HZPF) is a proposed instrument for the 10m class Hobby Eberly telescope that will be capable of discovering low mass planets around M dwarfs. HZPF will be fiber-fed,
...