The Astrophysical Journal · 2004 · 82 citations · 17 references
Natural SciencesAstronomyPhysicsAstrophysicsObservational AstronomyStellar AstronomyStellar ObservationsStellar SpectroscopyEccentricityOrbital EccentricityOrbital PeriodOrbital Period DeterminationRadial Velocity MeasurementsSignal-to-noise RatioTelescope SchedulingTelescopes
We report the first detection of a planetary-mass companion to a star using the High Resolution Spectrograph (HRS) of the Hobby-Eberly Telescope (HET). The HET-HRS now gives routine radial velocity precision of 2-3 m/s for high SNR observations of quiescent stars. The planetary-mass companion to the metal-rich K0V star HD37605 has an orbital period of 54.23 days, an orbital eccentricity of 0.737, and a minimum mass of 2.84 Jupiter masses. The queue-scheduled operation of the Hobby-Eberly Telescope enabled us to discovery of this relatively short-period planet with a total observation time span of just two orbital periods. The ability of queue-scheduled large-aperture telescopes to respond quickly to interesting and important results demonstrates the power of this new approach in searching for extra-solar planets as well as in other ares of research requiring rapid response time critical observations.
17
Abundances of the elements: Meteoritic and solar
Edward Anders, N. Grevesse · Geochimica et Cosmochimica Acta · 1989 · 10.5K citations
ELODIE: A spectrograph for accurate radial velocity measurements
A. Baranne, D. Queloz, M. Mayor et al. · Astronomy and Astrophysics Supplement Series · 1996 · 1.4K citations · Full text
Natural Sciences, Astronomy, Physics +10
Six New Planets from the Keck Precision Velocity Survey
Steven S. Vogt, Geoffrey W. Marcy, R. Paul Butler et al. · The Astrophysical Journal · 2000 · 201 citations · Full text