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Stephen J. Edberg

Researcher at California Institute of Technology

Publications -  16
Citations -  221

Stephen J. Edberg is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Planetary system & Astrometry. The author has an hindex of 4, co-authored 16 publications receiving 209 citations. Previous affiliations of Stephen J. Edberg include Jet Propulsion Laboratory.

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Taking the Measure of the Universe: Precision Astrometry with SIM PlanetQuest

TL;DR: The Space Interferometry Mission PlanetQuest (SIM PlanetQuest) as discussed by the authors was the first interferometer designed for precision astrometry, achieving a parallax of about 4 μas on targets as faint as V = 20, and differential accuracy of 0.6 μas.
Journal ArticleDOI

Studying Earth in the New Millennium: NASA Jet Propulsion Laboratory's Contributions to Earth Science and Applications Space Agencies

TL;DR: The NASA Jet Propulsion Laboratory (JPL) is a national research facility that carries out cuttingedge earth science missions as mentioned in this paper, and is a pioneer in the use of remote sensing for science of the oceans, atmosphere and solid earth.
Journal ArticleDOI

Taking the Measure of the Universe: Precision Astrometry with SIM PlanetQuest

TL;DR: The Space Interferometry Mission PlanetQuest (SIM PlanetQuest) was selected in 2000 for the NASA Astrobiology Challenge and has been successfully used to search for planets with masses as small as an Earth orbiting in the 'habitable zone' around the nearest stars.

Taking the Measure of the Universe: Precision Astrometry with SIM Planetquest (Preprint)

TL;DR: The Space Interferometry Mission PlanetQuest (SIM PlanetQuest) as mentioned in this paper was selected in 2000 for the NASA Astro Interference Mission (SIFT) to search for planets with masses as small as an Earth orbiting in the "habitable zone".
Posted Content

Astrometric Detection of Earthlike Planets

TL;DR: Astrometry can detect rocky planets in a broad range of masses and orbital distances and measure their masses and three-dimensional orbital parameters, including eccentricity and inclination, to provide the properties of terrestrial planets as discussed by the authors.