Add to ORKGClose-in extrasolar giant planets may be directly detectable by theirreflected light, due to the proximity of the planet to the illuminating star.The spectrum of the system will contain a reflected light component that variesin amplitude and Doppler shift as the planet orbits the star. Intensivesearches for this effect have been carried out for only one extrasolar planetsystem, tau Boo. There exist several other attractive targets, including thetransiting planet system HD 209458
© 2020 The American Astronomical Society. This is an author-created, un-copyedited version of an art...
Due to their extremely small luminosity compared to the stars they orbit, planets outside our own So...
One of the outstanding scientific questions in astronomy is the frequency at which solar systems for...
The close-in extrasolar giant planets [CEGPs], $\ltorder$ 0.05 AU from their parent stars, may have ...
Over the last few years, many close orbiting ($\sim 0.05 A. U.) large mass planets ($\sim M_J$) of n...
Looking out to the vastness of the night sky, stargazers often ponder questions about the universe, ...
We have used a Doppler tomographic analysis to conduct a deep search for the starlight reflected fro...
Planned astronomical observatories of the 2020s will be capable of obtaining reflected light photome...
Using improved Doppler tomographic signal-analysis techniques, we have carried out a deep search for...
In data from three clear nights of echelle spectroscopy in 2000 October/November, and using improved...
During the past five years we have pursued the detection of extrasolar planets by the photometric tr...
Aims. We attempt to detect starlight reflected from the hot Jupiter orbiting the main-sequence star ...
NASA's Kepler Mission promises to detect transiting Earth-sized planets in the habitable zones of so...
We have used a doppler tomographic analysis to conduct a deep search for the starlight reflected fro...
Motivated by the possibility that a coronagraph will be put on the Wide-field Infrared Survey Telesc...
© 2020 The American Astronomical Society. This is an author-created, un-copyedited version of an art...
Due to their extremely small luminosity compared to the stars they orbit, planets outside our own So...
One of the outstanding scientific questions in astronomy is the frequency at which solar systems for...
The close-in extrasolar giant planets [CEGPs], $\ltorder$ 0.05 AU from their parent stars, may have ...
Over the last few years, many close orbiting ($\sim 0.05 A. U.) large mass planets ($\sim M_J$) of n...
Looking out to the vastness of the night sky, stargazers often ponder questions about the universe, ...
We have used a Doppler tomographic analysis to conduct a deep search for the starlight reflected fro...
Planned astronomical observatories of the 2020s will be capable of obtaining reflected light photome...
Using improved Doppler tomographic signal-analysis techniques, we have carried out a deep search for...
In data from three clear nights of echelle spectroscopy in 2000 October/November, and using improved...
During the past five years we have pursued the detection of extrasolar planets by the photometric tr...
Aims. We attempt to detect starlight reflected from the hot Jupiter orbiting the main-sequence star ...
NASA's Kepler Mission promises to detect transiting Earth-sized planets in the habitable zones of so...
We have used a doppler tomographic analysis to conduct a deep search for the starlight reflected fro...
Motivated by the possibility that a coronagraph will be put on the Wide-field Infrared Survey Telesc...
© 2020 The American Astronomical Society. This is an author-created, un-copyedited version of an art...
Due to their extremely small luminosity compared to the stars they orbit, planets outside our own So...
One of the outstanding scientific questions in astronomy is the frequency at which solar systems for...