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Related papers: Retired A Stars and Their Companions: Exoplanets O…

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Keck/HIRES precision radial velocities of HD 207832 indicate the presence of two Jovian-type planetary companions in Keplerian orbits around this G star. The planets have minimum masses of 0.56 and 0.73 Jupiter-masses with orbital periods…

Earth and Planetary Astrophysics · Physics 2015-06-05 Nader Haghighipour , R. Paul Butler , Eugenio J. Rivera , Gregory W. Henry , Steven S. Vogt

Analyses of exoplanet statistics suggest a trend of giant planet occurrence with host star mass, a clue to how planets like Jupiter form. One missing piece of the puzzle is the occurrence around late K dwarf stars (masses of 0.5-0.75Msun…

Earth and Planetary Astrophysics · Physics 2015-06-15 Eric Gaidos , Debra A. Fischer , Andrew W. Mann , Andrew W. Howard

Doppler-based planet surveys have shown that, besides metallicity, the planet occurrence is also correlated with stellar mass, increasing from M to F-A spectral types. However, it has recently been argued that the subgiants (which represent…

Solar and Stellar Astrophysics · Physics 2014-08-15 Luan Ghezzi , José Dias do Nascimento , John Asher Johnson

We report the detection of a substellar companion orbiting the G5 dwarf HD 16760 from the N2K sample. Precise Doppler measurements of the star from Subaru and Keck revealed a Keplerian velocity variation with a period of 466.47+-0.35 d, a…

Ten new low mass companions have emerged from the Keck precision Doppler velocity survey, with minimum (msini) masses ranging from 0.8 mjup to 0.34 msun. Five of these are planet candidates with msini < 12 mjup, two are brown dwarf…

For over 10 years, we have carried out a precise radial velocity (RV) survey to find substellar companions around evolved G,K-type stars to extend our knowledge of planet formation and evolution. We performed high precision RV measurements…

Solar and Stellar Astrophysics · Physics 2017-11-29 M. Yılmaz , B. Sato , I. Bikmaev , S. O. Selam , H. Izumiura , V. Keskin , E. Kambe , S. S. Melnikov , A. Galeev , İ. Özavcı , E. N. Irtuganov , R. Ya. Zhuchkov

Doppler velocity measurements from the Anglo-Australian Planet Search reveal planetary mass companions to HD23127, HD159868, and a possible second planetary companion to HD154857. These stars are all G dwarfs. The companions are all in…

We report results of a search for planets around 500 main sequence stars using the Keck high resolution spectrometer which has provided Doppler precision of 3 m/s during the past 3 yr. We report 6 new strong planet candidates having…

Astrophysics · Physics 2009-10-31 Steven S. Vogt , Geoffrey W. Marcy , R. Paul Butler , Kevin Apps

We present precision radial velocity (RV) data sets from Keck-HIRES and from Lick Observatory's new Automated Planet Finder Telescope and Levy Spectrometer on Mt. Hamilton that reveal a multiple-planet system orbiting the nearby, slightly…

We present new precision radial velocities and a three-planet Keplerian orbit fit for the V = 8.5, G5 V star HIP 14810. We began observing this star at Keck Observatory as part of the N2K Planet Search Project. Wright et al. (2007)…

A precise radial velocity survey conducted by a Korean-Japanese planet search program revealed a planetary companion around the intermediate-mass clump giant HD 100655. The radial velocity of the star exhibits a periodic Keplerian variation…

We have detected a 12 M$_{\rm Jup}$ planet orbiting in or near the habitable zone of a main-sequence A star via the pulsational phase shifts induced by orbital motion. The planet has an orbital period of $840\pm20$ d and an eccentricity of…

Solar and Stellar Astrophysics · Physics 2016-08-17 Simon J. Murphy , Timothy R. Bedding , Hiromoto Shibahashi

We report the detection of a double planetary system around the evolved intermediate-mass star HD 47366 from precise radial-velocity measurements at Okayama Astrophysical Observatory, Xinglong Station, and Australian Astronomical…

We present the discovery of 7 new planets and 8 planet candidates around subgiant stars, as additions to the known sample of planets around "retired A stars" (Johnson et al. 2006). Among these are the possible first 3-planet systems around…

Earth and Planetary Astrophysics · Physics 2019-04-03 Jacob K. Luhn , Fabienne A. Bastien , Jason T. Wright , John A. Johnson , Andrew W. Howard , Howard Isaacson

We investigate the masses of "retired A stars" using asteroseismic detections on seven low-luminosity red-giant and sub-giant stars observed by the NASA Kepler and K2 Missions. Our aim is to explore whether masses derived from spectroscopy…

We present results from our ongoing spectroscopic search for giant planets within 1 AU around a well-defined sample of metal-poor stars with HIRES on the Keck 1 telescope. We have achieved an rms radial velocity precision of $\sim 8$ m/s…

Astrophysics · Physics 2013-05-29 A. Sozzetti , D. W. Latham , G. Torres , R. P. Stefanik , A. P. Boss , B. W. Carney , J. B. Laird

We aim to detect and characterize substellar companions to K giant stars, to further our knowledge of planet formation and stellar evolution of intermediate-mass stars. For more than a decade we have used Doppler spectroscopy to acquire…

Earth and Planetary Astrophysics · Physics 2015-06-16 D. S. Mitchell , S. Reffert , T. Trifonov , A. Quirrenbach , D. A. Fischer

We present radial velocity measurements of two stars observed as part of the Lick Subgiants Planet Search and the Keck N2K survey. Variations in the radial velocities of both stars reveal the presence of Jupiter-mass exoplanets in highly…

We classified the reddest ($r-J>2.2$) stars observed by the NASA $Kepler$ mission into main sequence dwarf or evolved giant stars and determined the properties of 4216 M dwarfs based on a comparison of available photometry with that of…

Earth and Planetary Astrophysics · Physics 2016-02-24 E. Gaidos , A. W. Mann , A. L. Kraus , M. Ireland

Precision Doppler velocity measurements from the 3.9--m Anglo-Australian Telescope reveal a planet with a 6 year period orbiting the G5 dwarf HD 70642. The a = 3.3 AU orbit has a low eccentricity (e = 0.1), and the minimum (\msini) mass of…