Two New Planets from the Anglo-Australian Planet Search

By R. P. Butler, C. Tinney, G. Marcy, H. Jones, A. Penny, K. Apps. 2001

133 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/e11cdc6074d6e223414e027a9691dd5771eb62db

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In Astronomy and Astrophysics

Citations in the corpus

State of the Field: Extreme Precision Radial Velocities (2016, background): “UCLES on the AAT has concentrated on the same sample of 240 stars from 1998 to 2012, detecting more than 45 new planets orbiting these stars (Butler et al. 2001; Carter et al. 2003; Bailey et al. 2009; O’Toole et al. 2009; Tinney et al. 2011; Wittenmyer et al. 2014).”
The HARPS survey for southern extra-solar planets. II. A 14 Earth-masses exoplanet around μ Arae (2004, background): “…uncertainty (∼40 cm s−1), and from the stellar noise (∼80 cm s−1) that is not completely averaged on the nights with only 15 radial velocity measurements (Bouchy et al., in prep.). µAra was previously announced to harbor a giant planet in a long period (∼740 days) orbit (Butler et al. 2001).”
Spectroscopic metallicities for planet-host stars: Extending the samples (2005, background): “Amid the stars in this new volume-limited comparison sample there is HD 147513 and the very metal rich planet-host star HD 160691 (Butler et al. 2001; Santos et al. 2004a).”
The great escape: how exoplanets and smaller bodies desert dying stars (2011, background): “In the second category, examples are thought to include Gl 86 = HD 13445 (Queloz et al. 2000; Mugrauer & Neuhäuser 2005; Lagrange et al. 2006), HD 27442 (Butler et al. 2001; Chauvin et al. 2006), and HD 147513 (Mayor et al. 2004; Desidera & Barbieri 2007).”
Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog (2006, background): “Furthermore, all three planet-host subgiants with well-defined ages are in fact super-metal-rich: HD27442 ([Fe/H] = +0.39), HD38529 ([Fe/H] = +0.31) and HD177830 ([Fe/H] = +0.36).”
Planet Migration and Gap Formation by Tidally Induced Shocks (2001, background): “The recent discovery of extrasolar planets in orbits very close to their parent stars (Mayor & Queloz 1995; Marcy, Butler, & Vogt 2000; Vogt et al. 2000; Butler et al. 2001) has raised a number of questions about the formation mechanisms of such systems.”
The planet search programme at the ESO CES and HARPS - IV. The search for Jupiter analogues around solar-like stars (2012, methodology): “The signal was also seen by Naef et al. (2001) using the CORALIE spectrograph and by Butler et al. (2001) with the AAT.”
The CORALIE survey for southern extra-solar planets - IX. A 1.3-day period brown dwarf disguised as a planet (2002, methodology): “1 See e.g. obswww.unige.ch/∼udry/planet/planet.html tion of the line-of-sight with a precision of the order of 2- 3m s−1 (e.g. Queloz et al. 2001a; Butler et al. 2001; Pepe et al. 2002), but even higher precision is expected from instruments available in the near future (e.g. HARPS – Pepe et al.…”