The Planet-Metallicity Correlation

@article{Fischer2005ThePC,
  title={The Planet-Metallicity Correlation},
  author={D. Fischer and J. Valenti},
  journal={The Astrophysical Journal},
  year={2005},
  volume={622},
  pages={1102-1117}
}
We have recently carried out spectral synthesis modeling to determine Teff, log g, v sin i, and [Fe/H] for 1040 FGK-type stars on the Keck, Lick, and Anglo-Australian Telescope planet search programs. This is the first time that a single, uniform spectroscopic analysis has been made for every star on a large Doppler planet search survey. We identify a subset of 850 stars that have Doppler observations sufficient to detect uniformly all planets with radial velocity semiamplitudes K > 30 m s-1… Expand
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The Metallicities of Stars With and Without Transiting Planets
The California-Kepler Survey. IV. Metal-rich Stars Host a Greater Diversity of Planets
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ARE STARS WITH PLANETS ANOMALOUS
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