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Giant Planets around FGK Stars Probably Form through Core Accretion
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A Physically Motivated and Empirically Calibrated Method to Measure the Effective Temperature, Metallicity, and Ti Abundance of M Dwarfs
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The AMBRE project: chemical evolution models for the Milky Way thick and thin discs
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Precise masses for the transiting planetary system HD 106315 with HARPS
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SPECTRAL PROPERTIES OF COOL STARS: EXTENDED ABUNDANCE ANALYSIS OF 1,617 PLANET-SEARCH STARS
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DISCOVERY AND VALIDATION OF A HIGH-DENSITY SUB-NEPTUNE FROM THE K2 MISSION
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