@article{03417c1f40f74321a0a02831942cd661,
title = "The California-Kepler Survey. II. Precise Physical Properties of 2025 Kepler Planets and Their Host Stars",
abstract = "We present stellar and planetary properties for 1305 Kepler Objects of Interest hosting 2025 planet candidates observed as part of the California-Kepler Survey. We combine spectroscopic constraints, presented in Paper I, with stellar interior modeling to estimate stellar masses, radii, and ages. Stellar radii are typically constrained to 11%, compared to 40% when only photometric constraints are used. Stellar masses are constrained to 4%, and ages are constrained to 30%. We verify the integrity of the stellar parameters through comparisons with asteroseismic studies and Gaia parallaxes. We also recompute planetary radii for 2025 planet candidates. Because knowledge of planetary radii is often limited by uncertainties in stellar size, we improve the uncertainties in planet radii from typically 42% to 12%. We also leverage improved knowledge of stellar effective temperature to recompute incident stellar fluxes for the planets, now precise to 21%, compared to a factor of two when derived from photometry.",
keywords = "planets and satellites: fundamental parameters, planets and satellites: general, stars: abundances, stars: fundamental parameters, techniques: spectroscopic",
author = "Johnson, {John Asher} and Petigura, {Erik A.} and Fulton, {Benjamin J.} and Marcy, {Geoffrey W.} and Howard, {Andrew W.} and Howard Isaacson and Leslie Hebb and Cargile, {Phillip A.} and Morton, {Timothy D.} and Weiss, {Lauren M.} and Winn, {Joshua N.} and Rogers, {Leslie A.} and Evan Sinukoff and Hirsch, {Lea A.}",
note = "Funding Information: We thank Jason Rowe, Dan Huber, and Jeff Valenti 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. 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 here are based on spectra 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 Followup 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. 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 NSF grant AST-1109612. L.H. acknowledges NSF grant AST-1009810. L.M.W. acknowledges support from Gloria and Ken Levy and from the the Trottier Family. E.S. is supported by a post- Funding Information: graduate scholarship from the Natural Sciences and Engineering Research Council of Canada. 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. This work has made use of data from the European Space Agency (ESA) mission Gaia, processed by the Gaia Data Processing and Analysis Consortium. Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. Publisher Copyright: {\textcopyright} 2017. The American Astronomical Society. All rights reserved.",
year = "2017",
month = sep,
doi = "10.3847/1538-3881/aa80e7",
language = "English (US)",
volume = "154",
journal = "Astronomical Journal",
issn = "0004-6256",
publisher = "IOP Publishing Ltd.",
number = "3",
}