The Transiting Exoplanet Survey Satellite

@inproceedings{Ricker2016TheTE,
  title={The Transiting Exoplanet Survey Satellite},
  author={George R. Ricker and Roland K. Vanderspek and Joshua N. Winn and Sara Seager and Zachory K. Berta-Thompson and Adam Levine and Joel S. Villasenor and David W. Latham and David Charbonneau and Matthew J. Holman and J. A. Johnson and Dimitar D. Sasselov and Andrew Szentgyorgyi and Guillermo Torres and G'asp'ar 'A. Bakos and Timothy M. Brown and J. Christensen-Dalsgaard and Hans Kjeldsen and Mark C. Clampin and Stephen Andrew Rinehart and Drake L. Deming and John P. Doty and Edward T. Dunham and Shigeru Ida and Nobuyuki Kawai and Bun’ei Sato and Jennifer M. Jenkins and Jack J. Lissauer and Garrett Jernigan and Lisa Kaltenegger and Gregory Laughlin and Douglas N. C. Lin and Peter Rankin McCullough and Norio Narita and Joshua A. Pepper and Keivan G. Stassun and St{\'e}phane Udry},
  booktitle={Astronomical Telescopes + Instrumentation},
  year={2016}
}
The Transiting Exoplanet Survey Satellite (TESS ) will search the solar neighborhood for planets transiting bright stars. TESS has been selected by NASA for launch in 2017 as an Astrophysics Explorer mission. The spacecraft will be placed into a highly elliptical 13.7-day orbit around the Earth. During its two-year mission, TESS will employ four wide-field optical CCD cameras to monitor at least 200,000 main-sequence dwarf stars with IC 13 for temporary drops in brightness caused by planetary… Expand
Transiting Exoplanet Survey Satellite
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Fine-pointing performance and corresponding photometric precision of the Transiting Exoplanet Survey Satellite
  • T. Nguyen, E. Morgan, +6 authors G. Ricker
  • Engineering, Computer Science
  • Journal of Astronomical Telescopes, Instruments, and Systems
  • 2018
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References

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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 ExplorerExpand
The Transiting Exoplanet Survey Satellite: Simulations of planet detections and astrophysical false positives
The Transiting Exoplanet Survey Satellite (TESS) is a NASA-sponsored Explorer mission that will perform a wide-field survey for planets that transit bright host stars. Here, we predict the propertiesExpand
A super-Earth transiting a nearby low-mass star
TLDR
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. Expand
TRAPPIST: TRAnsiting Planets and PlanetesImals Small Telescope
TRAPPIST is a 60-cm robotic telescope that has been installed in June 2010 at the ESO La Silla Observatory [1]. Operated from Liège (Belgium) it is devoted to the detection and characterisation ofExpand
Temperate Earth-sized planets transiting a nearby ultracool dwarf star
TLDR
Observations of three short-period Earth-sized planets transiting an ultracool dwarf star only 12 parsecs away suggest that 11 orbits remain possible for the third planet, the most likely resulting in irradiation significantly less than that received by Earth. Expand
Using All-Sky Surveys to Find Planetary Transits
Transits of bright stars offer a unique opportunity to study detailed properties of extrasolar planets that cannot be determined through radial-velocity observations. We propose a new technique toExpand
The MEarth-North and MEarth-South transit surveys: searching for habitable super-Earth exoplanets around nearby M-dwarfs
Detection and characterization of potentially habitable Earth-size extrasolar planets is one of the major goals of contemporary astronomy. By applying the transit method to very low-mass M-dwarfs, itExpand
Masses, Radii, and Orbits of Small Kepler Planets: The Transition From Gaseous to Rocky Planets
We report on the masses, sizes, and orbits of the planets orbiting 22 Kepler stars. There are 49 planet candidates around these stars, including 42 detected through transits and 7 revealed by preciseExpand
ExTrA: Exoplanets in transit and their atmospheres
The ExTrA facility, located at La Silla observatory, will consist of a near-infrared multi-object spectrograph fed by three 60-cm telescopes. ExTrA will add the spectroscopic resolution to theExpand
APF-The Lick Observatory Automated Planet Finder
AbstractThe Automated Planet Finder (APF) is a facility purpose-built for the discovery and characterization of extrasolar planets through high-cadence Doppler velocimetry of the reflex barycentricExpand
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