EPJ Web Conf.
Volume 160, 2017Seismology of the Sun and the Distant Stars 2016 – Using Today’s Successes to Prepare the Future – TASC2 & KASC9 Workshop – SPACEINN & HELAS8 Conference
|Number of page(s)||3|
|Section||Space Missions, Data and Projects|
|Published online||27 October 2017|
LAMOST observations in the K2 fields: project and observation progress
Department of Astronomy, Beijing Normal University, Beijing, 100875, China
2 Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030 China
3 National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing 100012 China
* e-mail: email@example.com
Published online: 27 October 2017
To complement the time-series observations of the Kepler space mission in the K2 fields, spectroscopic observations for hundreds of thousands of stars in these fields are hugely important. LAMOST, a Chinese 4-meter class telescope equipped with 4000 fibers on the focal plane, is an ideal facility to fulfill this task. The LAMOST-K2 project was approved in the autumn of 2015 and observations commenced during the 2015-2016 winter season. The project will initially cover 6 of the first 10 observed K2 campaigns, and may be extended to include later K2 campaigns. We describe the project and introduce the current progress of observation with this poster presentation.
© Owned by the authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).
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