190 datasets found

Keywords: g stars

Filter Results
  • Lithium abundances of a large sample of red giants

    The lithium abundances for 378 G/K giants are derived with non-local thermodynamic equilibrium correction considered. Among these are 23 stars that host planetary systems. The...
  • Oxygen abundances in nearby FGK stars

    Atmospheric parameters and oxygen abundances of 825 nearby FGK stars are derived using high-quality spectra and a non-local thermodynamic equilibrium analysis of the 777nm OI...
  • Lithium abundances in HIP stars

    We derive atmospheric parameters and lithium abundances for 671 stars and include our measurements in a literature compilation of 1381 dwarf and subgiant stars. First, a...
  • A search for new companions with CHARA

    We present the results of a comprehensive search for new companions to nearby solar-type stars using the separated fringe packet (SFP) technique at the Center for High Angular...
  • Abundances in G-type stars with exoplanets

    We confirm the difference in chemical abundance between stars with and without exoplanets and present the relation between chemical abundances and physical properties of...
  • Follow-up photometry of HAT-P-27

    We report the discovery of HAT-P-27b, an exoplanet transiting the moderately bright G8 dwarf star GSC 0333-00351 (V=12.214). The orbital period is 3.039586+/-0.000012 days, the...
  • Orbital eccentricities of 31535 G-dwarfs

    We test four competing models that aim to explain the nature of stars in spiral galaxies that are well away (>1kpc) from the midplane, the so-called thick disk: the stars may...
  • Stellar X-ray sources in the COSMOS survey

    We present an analysis of the X-ray properties of a sample of solar- and late-type field stars identified in the Chandra Cosmic Evolution Survey (COSMOS), a deep (160ks) and...
  • Follow-up observations of HAT-P-15

    We report the discovery of HAT-P-15b, a transiting extrasolar planet in the "period valley," a relatively sparsely populated period regime of the known extrasolar planets. The...
  • Abundances of solar analogs with planets

    We present a fully differential chemical abundance analysis using very high resolution ({lambda}/{delta}{lambda}>~85000) and very high signal-to-noise (S/N~800 on average)...
  • Chemical composition of OGLE-2007-BLG-514S

    We present a high-resolution spectrum of a microlensed G dwarf in the Galactic bulge with spectroscopic temperature T_eff_=5600+/-180K. This I~21mag star was magnified by a...
  • Radial velocities for 61 Vir

    We present precision radial velocity data that reveal a multiple exoplanet system orbiting the bright nearby G5V star 61 Virginis. Our 4.6 years of combined Keck/HIRES and...
  • IRS spectra of solar-type stars

    We have observed 152 nearby solar-type stars with the Infrared Spectrometer (IRS) on the Spitzer Space Telescope. Including stars that met our criteria but were observed in...
  • Age estimation for solar-type dwarfs

    While the strong anticorrelation between chromospheric activity and age has led to the common use of the CaII H and K emission index (R'HK=L_HK_/L_bol_) as an empirical age...
  • 25yr CaII-HK observations of F-K nearby stars

    We find a significant correlation between the magnetic and rotational moments for a sample of 112 lower main-sequence stars. The rotational moment is calculated from...
  • Absolute Calibration. IV. Templates for bright stars

    We demonstrate an approach to determine spectral energy distribution (SED) templates that are accurate to the 1% level from the visible through the infrared for nearby...
  • JWST MIRI spectrum of T Cha

    Understanding when and how circumstellar disks disperse is crucial to constrain planet formation and migration. Thermal winds powered by high-energy stellar photons have long...
  • Radial velocity follow up of HD 307842

    We report the confirmation of a TESS-discovered transiting super-Earth planet orbiting a mid-G star, HD307842 (TOI-784). The planet has a period of 2.8days, and the radial...
  • HARPS-N and NEID radial velocities of TOI-1420

    We present the discovery of TOI-1420b, an exceptionally low-density ({rho}=0.08{+/-}0.02g/cm^3^) transiting planet in a P=6.96days orbit around a late G-dwarf star. Using...
  • EXPRES radial volocity for {tau} Ceti

    To accurately characterize the planets a star may be hosting, stellar parameters must first be well determined. {tau}Ceti is a nearby solar analog and often a target for...
You can also access this registry using the API (see API Docs).