Journal
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Volume 169, Issue 2, Pages 430-438Publisher
IOP PUBLISHING LTD
DOI: 10.1086/513108
Keywords
methods : statistical; planetary systems; stars : abundances
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We report high-precision atmospheric parameters for 1907 stars in the N2K low-resolution spectroscopic survey, designed to identify metal-rich FGK dwarfs likely to harbor detectable planets. Of these stars, 284 are in the ideal temperature range for planet searches, T-eff <= 6000 K, and have a 10% or greater probability of hosting planets based on their metallicities. The stars in the low-resolution spectroscopic survey should eventually yield >60 new planets, including 8- hot Jupiters. Short-period planets have already been discovered orbiting the survey targets HIP 14810 and HD 149143.
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