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    • 域名年龄:24年8天  注册日期:2000年11月02日  到期时间:
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      注册商:Hichina Zhicheng Technology Limited 
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      主办单位:中国科学院国家天文台  性质:事业单位
      网站名:中国科学院国家天文台郭守敬望远镜网站  首页网址:www.lamost.org 
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    lamost.org

    域名年龄: 24年8天
    注册时间: 2000-11-02
    注 册 商: Hichina Zhicheng Technology Limited
    注册邮箱: ccz
    联系电话: +86.1064872500

    获取时间: 2016年12月26日 21:13:00
    Domain Name: LAMOST.ORG
    Domain ID: D39641512-LROR
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    Referral URL: http://www.net.cn
    Updated Date: 2016-10-16T08:24:54Z
    Creation Date: 2000-11-02T03:41:05Z
    Registry Expiry Date: 2025-11-02T03:41:05Z
    Sponsoring Registrar: Hichina Zhicheng Technology Limited
    Sponsoring Registrar IANA ID: 420
    Domain Status: ok https://icann.org/epp#ok
    Registrant ID: HC-049402250-CN
    Registrant Name: Cui Chenzhou
    Registrant Organization: National Astronomical Observatories, CAS
    Registrant Street: 20A Datun Road, Chaoyang district, Beijing 100012, China
    Registrant City: Beijing
    Registrant State/Province: Beijing
    Registrant Postal Code: 100012
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    Admin ID: HC-086933091-CN
    Admin Name: Cui Chenzhou
    Admin Organization: National Astronomical Observatories, CAS
    Admin Street: 20A Datun Road, Chaoyang District, Beijing 100012, China
    Admin City: Beijing
    Admin State/Province: Beijing
    Admin Postal Code: 100012
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    Tech ID: HC-366722633-CN
    Tech Name: Cui Chenzhou
    Tech Organization: Cui Chen Zhou
    Tech Street: 20A Datun Road, Chaoyang District, Beijing 100012, China
    Tech City: Beijing
    Tech State/Province: Beijing
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    Tech Country: CN
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    Name Server: DNS9.HICHINA.COM
    Name Server: DNS10.HICHINA.COM
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    抓取时间:2015年06月21日 19:53:40
    网址:http://dixie.lamost.org/
    标题:LAMOST
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    Sky Survey
    Telescope
    LAMOST PDR
    LAMOST DR1
    LAMOST DR2
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    LAMOST 973
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    LAMOST Survey
    LAMOST survey contains two main parts: the LAMOST ExtraGAlactic Survey (LEGAS), and the LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) survey of Milky Way stellar structure. The unique design of LAMOST enables it to take 4000 spectra in a single exposure to a limiting magnitude as faint as r=19 at the resolution R=1800, which is equivalent to the design aim of r=20 for the resolution R=500. This telescope therefore has great potential to efficiently survey a large volume of space for stars and galaxies.
    More
    News
    Spectroscopic analysis of metal-poor stars from LAMOST: early results  
    The velocity distribution in the solar neighborhood from the LAMOST pilot survey  
    White dwarf-main sequence binaries from LAMOST: the DR1 catalogues  
    The Nearest High Velocity Stars Revealed by LAMOST Data Release 1  
    Nearest Bright 'Hypervelocity Star' Found
    More News
    Survey Policy
    LAMOST Spectral Survey Data Policy
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    Copyright 1997-2012 LAMOST, National Astronomical Observatories, China

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