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The LAMOST Complete Spectroscopic Survey of Pointing Area at Southern Galactic Cap

机译:南银帽指向区域的拉米电池完整的光谱调查

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The LAMOST Complete Spectroscopic Survey of Pointing Area (LCSSPA) at Southern Galactic Cap (SGC). is one of the LAMOST Key Project, designed to complete the spectroscopic observations of all Galactic and extra-galactic sources in two selected fields of 20 degrees~2 at SGC, with the limiting magnitude of r= 18.1 mag. The main purposes of the project are focused on the completeness of the LAMOST ExtraGAlactic Surveys (LEGAS), testing the selection methods of galaxies and stars, and obtaining the basic performance parameters of the LAMOST telescope. Meanwhile the scientific studies include galaxies, clusters of galaxies, variable sources (quasars and variable stars), infrared excess stars and luminous infrared galaxies. The project has considerable scientific value since it is the most complete spectral data in LEGAS up to now. The project completed its observation in the early of 2014, and obtained at least 5000 spectra of galaxies and 25000 spectra of stars.
机译:南银帽(SGC)指向区域(LCSSPA)的拉米电池完整光谱勘探。是其中一个拉莫斯蒂钥匙项目,旨在在SGC的两个选定场中完成所有银河系和外层源的光谱观察,r = 18.1 mag的限制幅度。该项目的主要目的主要集中在拉米骨底胶调查(LEGAS)的完整性,测试星系和恒星的选择方法,并获得拉米镜子望远镜的基本性能参数。同时,科学研究包括星系,星系集群,可变源(Quasars和可变星星),红外线多恒星和发光红外星系。该项目具有相当大的科学价值,因为它是Legas中最完整的频谱数据到目前为止。该项目在2014年初完成了观察,并获得了至少5000个星系光谱和25000个星星光谱。

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