000002699 001__ 2699
000002699 005__ 20160701171709.0
000002699 0247_ $$2DOI$$a10.1051/epjconf/201510101011
000002699 037__ $$aASTROimport-856
000002699 100__ $$aDe Cat, P.
000002699 245__ $$aLAMOST observations in the Kepler field
000002699 260__ $$c2015
000002699 520__ $$aThe Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) at the Xinglong observatory in China is a new 4-m telescope equipped with 4,000 optical fibers. In 2010, we initiated the LAMOST-Kepler project. We requested to observe the full field-of-view of the nominal Kepler mission with the LAMOST to collect low-resolution spectra for as many objects from the KIC 10 catalogue as possible. So far, 12 of the 14 requested LAMOST fields have been observed resulting in more than 68,000 low-resolution spectra. Our preliminary results show that the stellar parameters derived from the LAMOST spectra are in good agreement with those found in the literature based on high-resolution spectroscopy. The LAMOST data allows to distinguish dwarfs from giants and can provide the projected rotational velocity for very fast rotators. 
000002699 700__ $$a Fu, J. N.
000002699 700__ $$a Yang, X. H.
000002699 700__ $$a Ren, A. B.
000002699 700__ $$a Frasca, A.
000002699 700__ $$a Molenda-Zakowicz, J.
000002699 700__ $$a Catanzaro, G.
000002699 700__ $$a Gray, R. O.
000002699 700__ $$a Corbally, C. J.
000002699 700__ $$a Shi, J. R.
000002699 700__ $$a Zhang, H. T.
000002699 700__ $$a Luo, A. L.
000002699 773__ $$c01011$$pEuropean Physical Journal Web of Conferences$$v101$$y2015
000002699 85642 $$ahttp://esoads.eso.org/abs/2015EPJWC.10101011D
000002699 905__ $$apublished in
000002699 980__ $$aNONREF