31 July 2017 to 3 August 2017
Royal Observatory of Belgium
UTC timezone
<br>2nd LAMOST-Kepler workshop<br><br>LAMOST in the era of large spectroscopic surveys<P><img src="https://events.oma.be/indico/event/26/picture/0.jpg" width="466" height="50">

Session

1 Current Status of the LAMOST and the LAMOST-Kepler Project

1
31 Jul 2017, 11:00
Meridian Room (Royal Observatory of Belgium)

Meridian Room

Royal Observatory of Belgium

Av. Circulaire - 3 - Ringlaan 1180 Brussels

Presentation materials

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  1. Dr Haotong Zhang (National Astronomical observatories of China, CAS)
    31/07/2017, 11:00
    1 Current Status of the LAMOST and the LAMOST-Kepler Project
    Invited Review
    I will review the current status of LAMOST Survey Strategy System(SSS) and the 2D data reduction pipeline. LAMOST SSS is a pipeline to allocate the fibers to the targets on the sky, it is designed to obtain the best survey efficiency, considering the limitation of the telescope and user requirement(such as the object priority). LAMOST SSS has been working steadily for five years, most of the...
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  2. Prof. Jianrong Shi (National Astronomical Observatories, Chinese Academy of Sciences)
    31/07/2017, 11:40
    1 Current Status of the LAMOST and the LAMOST-Kepler Project
    Invited Review
    I will introduce the observations of the LAMOST survey, the magnitudes and exposure times of the VB, V, B, M and F plates. I will also present some test observations of medium resolution spectra, and will describe the future medium resolution survey.
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  3. Prof. Ali Luo (National Astronomical Observatories, Chinese Academy of Scienes)
    31/07/2017, 12:20
    1 Current Status of the LAMOST and the LAMOST-Kepler Project
    Invited Review
    In this talk, a review of the current status of data reduction pipeline of LAMOST and an overview of the updates to the 2D and 1D reduction procedures and the LAMOST stellar parameter pipeline (LASP) will be given. The different versions of the data releases will be compared, the access to the data will be introduced and the details of the data quality will be presented. Stellar parameters are...
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