000002092 001__ 2092
000002092 005__ 20160701171658.0
000002092 0247_ $$2DOI$$a10.3847/0004-6256/151/1/13
000002092 037__ $$aASTROimport-249
000002092 100__ $$aGray, R. O.
000002092 245__ $$aLAMOST Observations in the Kepler Field: Spectral Classification with the MKCLASS Code
000002092 260__ $$c2016
000002092 520__ $$aThe LAMOST-Kepler project was designed to obtain high-quality, low-resolution spectra of many of the stars in the Kepler field with the Large Sky Area Multi Object Fiber Spectroscopic Telescope (LAMOST) spectroscopic telescope. To date 101,086 spectra of 80,447 objects over the entire Kepler field have been acquired. Physical parameters, radial velocities, and rotational velocities of these stars will be reported in other papers. In this paper we present MK spectral classifications for these spectra determined with the automatic classification code MKCLASS. We discuss the quality and reliability of the spectral types and present histograms showing the frequency of the spectral types in the main table organized according to luminosity class. Finally, as examples of the use of this spectral database, we compute the proportion of A-type stars that are Am stars, and identify 32 new barium dwarf candidates. 
000002092 700__ $$a Corbally, C. J.
000002092 700__ $$a De Cat, P.
000002092 700__ $$a Fu, J. N.
000002092 700__ $$a Ren, A. B.
000002092 700__ $$a Shi, J. R.
000002092 700__ $$a Luo, A. L.
000002092 700__ $$a Zhang, H. T.
000002092 700__ $$a Wu, Y.
000002092 700__ $$a Cao, Z.
000002092 700__ $$a Li, G.
000002092 700__ $$a Zhang, Y.
000002092 700__ $$a Hou, Y.
000002092 700__ $$a Wang, Y.
000002092 773__ $$c13$$i1$$pThe Astronomical Journal$$v151$$y2016
000002092 85642 $$ahttp://esoads.eso.org/abs/2016AJ....151...13G
000002092 905__ $$apublished in
000002092 980__ $$aREFERD