THE SEGUE STELLAR PARAMETER PIPELINE. I. DESCRIPTION AND COMPARISON OF INDIVIDUAL METHODS
文献类型：期刊论文
| 作者 | Lee, Young Sun1,2; Beers, Timothy C.1,2; Sivarani, Thirupathi1,2; Prieto, Carlos Allende3; Koesterke, Lars3; Wilhelm, Ronald4; Fiorentin, Paola Re5; Bailer-Jones, Coryn A. L.5; Norris, John E.6; Rockosi, Constance M.7 |
| 刊名 | ASTRONOMICAL JOURNAL
 |
| 出版日期 | 2008-11-01 |
| 卷号 | 136期号:5页码:2022-2049 |
| 关键词 | methods: data analysis stars: abundances stars: fundamental parameters surveys techniques: spectroscopic |
| 英文摘要 | We describe the development and implementation of the Sloan Extension for Galactic Exploration and Understanding (SEGUE) Stellar Parameter Pipeline (SSPP). The SSPP is derived, using multiple techniques, radial velocities, and the fundamental stellar atmospheric parameters (effective temperature, surface gravity, and metallicity) for AFGK-type stars, based on medium-resolution spectroscopy and ugriz photometry obtained during the course of the original Sloan Digital Sky Survey (SDSS-I) and its Galactic extension (SDSS-II/SEGUE). The SSPP also provides spectral classification for a much wider range of stars, including stars with temperatures outside the window where atmospheric parameters can be estimated with the current approaches. This is Paper I in a series of papers on the SSPP; it provides an overview of the SSPP, and tests of its performance using several external data sets. Random and systematic errors are critically examined for the current version of the SSPP, which has been used for the sixth public data release of the SDSS (DR-6). |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000260132500025 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/7421]  |
| 专题 | 国家天文台_光学天文研究部 |
| 作者单位 | 1.Michigan State Univ, Dept Phys & Astron, CSCE, E Lansing, MI 48824 USA 2.Michigan State Univ, Joint Inst Nucl Astrophys, E Lansing, MI 48824 USA 3.Univ Texas Austin, Dept Astron, Austin, TX 78712 USA 4.Texas Tech Univ, Dept Phys, Lubbock, TX 79409 USA 5.Max Planck Inst Astron, D-69117 Heidelberg, Germany 6.Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia 7.Univ Calif Santa Cruz, Dept Astron, Santa Cruz, CA 95064 USA 8.Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA 9.Rensselaer Polytech Inst, Dept Phys & Astron, Troy, NY 12180 USA 10.Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA |
| 推荐引用方式 GB/T 7714 | Lee, Young Sun,Beers, Timothy C.,Sivarani, Thirupathi,et al. THE SEGUE STELLAR PARAMETER PIPELINE. I. DESCRIPTION AND COMPARISON OF INDIVIDUAL METHODS[J]. ASTRONOMICAL JOURNAL,2008,136(5):2022-2049. |
| APA | Lee, Young Sun.,Beers, Timothy C..,Sivarani, Thirupathi.,Prieto, Carlos Allende.,Koesterke, Lars.,...&Luo, A. -Li.(2008).THE SEGUE STELLAR PARAMETER PIPELINE. I. DESCRIPTION AND COMPARISON OF INDIVIDUAL METHODS.ASTRONOMICAL JOURNAL,136(5),2022-2049. |
| MLA | Lee, Young Sun,et al."THE SEGUE STELLAR PARAMETER PIPELINE. I. DESCRIPTION AND COMPARISON OF INDIVIDUAL METHODS".ASTRONOMICAL JOURNAL 136.5(2008):2022-2049. |
入库方式： OAI收割
来源：国家天文台
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