2016/06/29 by A. Frasca, J. Molenda-Zakowicz, J. Molenda‐Żakowicz +13
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Kepler #LAMOST #Physics #Spectral line #Spitzer Space Telescope #Stars #Stellar, planetary, and galactic studies #Telescope #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201628337
published as A&A 594, A39 (2016) · A&A accepted, 16 pages, 18 figures, 3 appendices
arxiv created 2016/06/29 · openalex publication_date 2016/07/12 · arxiv updated 2016/10/07 · openalex created_date 2022/08/20 · openalex updated_date 2026/08/05
Aims. A comprehensive and homogeneous determination of stellar parameters for the stars observed by the Kepler space telescope is necessary for statistical studies of their properties. As a result of the large number of stars monitored by Kepler, the largest and more complete databases of stellar parameters published to date are multiband photometric surveys. The LAMOST-Kepler survey, whose spectra are analyzed in the present paper, was the first large spectroscopic project, which started in 2011 and aimed at filling that gap. In this work we present the results of our analysis, which is focused on selecting spectra with emission lines and chromospherically active stars by means of the spectral subtraction of inactive templates. The spectroscopic determination of the atmospheric parameters for a large number of stars is a by-product of our analysis.