{ "id": "1411.0913", "version": "v1", "published": "2014-11-04T14:00:25.000Z", "updated": "2014-11-04T14:00:25.000Z", "title": "LAMOST observations in the Kepler field", "authors": [ "Peter De Cat", "Jianning Fu", "Xiaohu Yang", "Anbing Ren", "Antonio Frasca", "Joanna Molenda-Żakowicz", "Giovanni Catanzaro", "Richard O. Gray", "Chris J. Corbally", "Jianrong Shi", "Haotong Zhang", "Ali Luo" ], "comment": "CoRoT Symposium 3 / Kepler KASC-7 joint meeting, Toulouse, July 2014. To be published by EPJ Web of Conferences", "categories": [ "astro-ph.SR" ], "abstract": "The 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 KIC10 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.", "revisions": [ { "version": "v1", "updated": "2014-11-04T14:00:25.000Z" } ], "analyses": { "keywords": [ "kepler field", "lamost observations", "large sky area multi-object fiber", "area multi-object fiber spectroscopic telescope", "sky area multi-object fiber spectroscopic" ], "publication": { "doi": "10.1051/epjconf/201510101011" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1326051, "adsabs": "2015EPJWC.10101011D" } } }