A Planetary Companion to the Hyades Giant ϵ Tauri

By Bun'ei Sato, H. Izumiura, E. Toyota, E. Kambe, Y. Takeda, S. Masuda, M. Omiya, D. Murata, Y. Itoh, H. Ando and 4 more. 2007

139 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/505f08767c94b32af00dd96b7710c06aa90d72d6

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In Astronomy and Astrophysics

1. C. Lovis
2. M. Mayor
3. S. Reffert
4. K. Ulaczyk
5. T. Sumi
6. M. Szymański
7. T. Trifonov
8. A. Udalski

Citations in the corpus

• Precise Radial Velocities of Giant Stars VII. Occurrence Rate of Giant Extrasolar Planets as a Function of Mass and Metallicity (2014, background): “Eight of the 15 systems with a secure planet in our Lick sample have been published already: ι Dra b (Frink et al. 2002), Pollux b (Reffert et al. 2006; Hatzes et al. 2006), ε Tau b (Sato et al. 2007), 11 Com b (Liu et al. 2008), ν Oph b and c (Quirrenbach et al. 2011; Sato et al. 2013), τ Gem b and”
• THE ORBITAL EVOLUTION OF GAS GIANT PLANETS AROUND GIANT STARS (2009, unknown): “…more-massive stars in an evolved stage (Döllinger et al. 2007, 2009; Frink et al. 2002; Hatzes et al. 2003, 2005, 2006; Johnson et al. 2007a, 2007b, 2008; Liu et al. 2007; Lovis & Mayor 2007; Niedzielski et al. 2007, 2009; Reffert et al. 2006; Sato et al. 2007, 2008; Setiawan et al. 2003, 2005).”
• Precise radial velocities of giant stars. III. Spectroscopic stellar parameters (2007, unknown): “0 dex for Mishenina et al. (2006), −0.05 dex for Sadakane et al. (2005), Sato et al. (2007) and Takeda et al. (2005), and−0.85 dex for Twarog et al. (1997).”
• Stellar Parameters and Elemental Abundances of Late-G Giants (2008, unknown): “…10 stars (out of 322 objects) as stars hosting planets: HD 104985 (Sato et al. 2003); HD 62509 (Reffert et al. 2006; Hatzes et al. 2006); HD 28305 (Sato et al. 2007); HD 142091, HD 167042, and HD 210702 (Johnson et al. 2007; Sato et al., in preparation); HD 1073832 (Liu et al. 2008); HD 81688, HD…”
• Planets around evolved intermediate-mass stars - I. Two substellar companions in the open clusters NGC 2423 and NGC 4349 (2007, background): “With the recent discovery by Sato et al. (2007), we now have 3 massive planets or brown dwarfs orbiting intermediate-mass stars in open clusters.”
• A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192 (2008, background): “Gas giant planets have been found in orbit around stars of all these types (Butler et al. 2006; Sato et al. 2007; Johnson et al. 2007; Niedzielski et al. 2007; Lovis & Mayor 2007), but they appear to be increasingly rare in orbit around low-mass stars.”