@article{b242cb45ddcb45e79b6fc94d3fa972de,
title = "The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets",
abstract = "The California-Kepler Survey (CKS) is an observational program developed to improve our knowledge of the properties of stars found to host transiting planets by NASA's Kepler Mission. The improvement stems from new high-resolution optical spectra obtained using HIRES at the W. M. Keck Observatory. The CKS stellar sample comprises 1305 stars classified as Kepler objects of interest, hosting a total of 2075 transiting planets. The primary sample is magnitude-limited (Kp < 14.2) and contains 960 stars with 1385 planets. The sample was extended to include some fainter stars that host multiple planets, ultra-short period planets, or habitable zone planets. The spectroscopic parameters were determined with two different codes, one based on template matching and the other on direct spectral synthesis using radiative transfer. We demonstrate a precision of 60 K in Teff, 0.10 dex in log g, 0.04 dex in [Fe/H], and 1.0km s-1 in V sin i. In this paper, we describe the CKS project and present a uniform catalog of spectroscopic parameters. Subsequent papers in this series present catalogs of derived stellar properties such as mass, radius, and age; revised planet properties; and statistical explorations of the ensemble. CKS is the largest survey to determine the properties of Kepler stars using a uniform set of high-resolution, high signal-to-noise ratio spectra. The HIRES spectra are available to the community for independent analyses.",
keywords = "binaries: spectroscopic, catalogs, stars: abundances, stars: fundamental parameters",
author = "Petigura, {Erik A.} and Howard, {Andrew W.} and Marcy, {Geoffrey W.} and Johnson, {John Asher} and Howard Isaacson and Cargile, {Phillip A.} and Leslie Hebb and Fulton, {Benjamin J.} and Weiss, {Lauren M.} and Morton, {Timothy D.} and Winn, {Joshua N.} and Rogers, {Leslie A.} and Evan Sinukoff and Hirsch, {Lea A.} and Crossfield, {Ian J.M.}",
note = "Funding Information: We thank Jason Rowe, Dan Huber, Jeff Valenti, Natalie Batalha, and David Ciardi for helpful conversations and Roberto Sanchis-Ojeda for his work on the Ultra-Short Period planet sample. We thank the many observers who contributed to the measurements reported here. P.A.C. and L.H. thank Jeff Valenti and Eric Stempels for their extensive help in running SME and developing the SME implementation presented in this paper. We gratefully acknowledge the efforts and dedication of the Keck Observatory staff, especially Randy Campbell, Scott Dahm, Greg Doppmann, Marc Kassis, Jim Lyke, Hien Tran, Josh Walawender, and Greg Wirth for support with HIRES and with remote observing. Most of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA. We are grateful to the time assignment committees of the University of Hawaii, the University of California, the California Institute of Technology, and NASA for their generous allocations of observing time that enabled this large project. Kepler was competitively selected as the tenth NASA Discovery mission. Funding for this mission is provided by the NASA Science Mission Directorate. We thank the Kepler Science Office, the Science Operations Center, Threshold Crossing Event Review Team (TCERT), and the Follow-up Observations Program (FOP) Working Group for their work on all steps in the planet discovery process ranging from selecting target stars and pointing the Kepler telescope to developing and running the photometric pipeline to curating and refining the catalogs of Kepler planets. We specifically thank Natalie Batalha, William Borucki, and David Ciardi, in particular, for selecting stars in the Habitable Zone sample. E.A.P. acknowledges support from Hubble Fellowship grant HST-HF2-51365.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA under contract NAS 5-26555. A.W.H. acknowledges NASA grant NNX12AJ23G. T.D.M. acknowledges NASA grant NNX14AE11G. P.A.C. acknowledges National Science Foundation grant AST-1109612. L.H. acknowledges National Science Foundation grant AST-1009810. L.M.W. acknowledges support from Gloria and Ken Levy and from the Trottier Family. E.S. is supported by a post-graduate scholarship from the Natural Sciences and Engineering Research Council of Canada. I.J.M.C. performed his work under contract with the Jet Propulsion Laboratory (JPL) funded by NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute. Work by J.N.W. was partly supported by a NASA Keck PI Data Award, administered by the NASA Exoplanet Science Institute. This work made use of the SIMBAD database (operated at CDS, Strasbourg, France), NASA{\textquoteright}s Astrophysics Data System Bibliographic Services, and the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. L.A.R. gratefully acknowledges support provided by NASA through Hubble Fellowship grant #HF-51313 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. This work was performed in part under contract with the Jet Propulsion Laboratory (JPL) funded by NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute. Finally, the authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. Facilities: Keck:I (HIRES), Kepler. Publisher Copyright: {\textcopyright} 2017. The American Astronomical Society. All rights reserved.",
year = "2017",
month = sep,
doi = "10.3847/1538-3881/aa80de",
language = "English (US)",
volume = "154",
journal = "Astronomical Journal",
issn = "0004-6256",
publisher = "IOP Publishing Ltd.",
number = "3",
}