000003405 001__ 3405
000003405 005__ 20180116112337.0
000003405 0247_ $$2DOI$$a10.1051/epjconf/201715204002
000003405 037__ $$aSCART-2018-0018
000003405 100__ $$aMolenda-Żakowicz, J.
000003405 245__ $$aThe LAMOST spectroscopic survey of stars in the Kepler field of view: Activity indicators and stellar parameters
000003405 260__ $$c2017
000003405 520__ $$aWe summarize the results of the completed first round of the LAMOST-Kepler project, and describe the status of its on-going second round. As a result of the first round of this project, the atmospheric parameters (Teff, log g, and [Fe/H]), the spectral classification (spectral type and luminosity class), and the radial velocities (RV) have been measured for 51,385 stars. For 4031 stars, we were able to measure the projected rotational velocity, while the minimum detectable v sin i was 120 km s-1. For 8821 stars with more than one observation, we computed the χ-square probability that the detected RV variations have a random occurrence. Finally, we classified 442 stars as chromospherically active on the basis of the analysis of their Hα and Ca II-IRT fluxes. All our results have been obtained from the low-resolution (R ˜ 1800) spectroscopic observations acquired with the LAMOST instrument. Based on observations collected with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) located at the Xinglong Observatory, China.
000003405 594__ $$aNO
000003405 700__ $$aFrasca, A.
000003405 700__ $$aDe Cat, P.
000003405 700__ $$aCatanzaro, G.
000003405 773__ $$c1-5$$nid. 04002$$pEPJ Web of Conferences$$v152$$y2017
000003405 8560_ $$fpeter@observatoire.be
000003405 85642 $$ahttps://www.epj-conferences.org/articles/epjconf/abs/2017/21/epjconf_puls2017_04002/epjconf_puls2017_04002.html
000003405 8564_ $$s219360$$uhttp://publi2-as.oma.be/record/3405/files/MolendaŻakowicz2017_EPJWC152_04002.pdf
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000003405 905__ $$apublished in
000003405 980__ $$aNONREF