中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Oxygen Abundance Methods in SDSS: View from Modern Statistics

文献类型:期刊论文

作者Shi, Fei; Zhao, Gang; Wicker, James
刊名JOURNAL OF ASTROPHYSICS AND ASTRONOMY
出版日期2010-09-01
卷号31期号:3页码:121-133
关键词Galaxies: abundance, starburst stars: formation
英文摘要Our purpose is to find which is the most reliable one among various oxygen abundance determination methods. We will test the validity of several different oxygen abundance determination methods using methods of modem statistics. These methods include Bayesian analysis and information scoring. We will analyze a sample of similar to 6000 HII galaxies from the Sloan Digital Sky Survey (SDSS) spectroscopic observations data release four. All methods that we used drew the same conclusion that the T(e) method is a more reliable oxygen abundance determination method than the Bayesian metallicity method under the existing telescope ability. The ratios of the likelihoods between the different kinds of methods tell us that the Te, P, and O3N2 methods are consistent with each other because the P and O3N2 methods are calibrated by Te method. The Bayesian and R(23) methods are consistent with each other because both are calibrated by a galaxy model. In either case, the N2 method is an unreliable method.
收录类别SCI
语种英语
WOS记录号WOS:000282184900001
源URL[http://ir.bao.ac.cn/handle/114a11/7661]  
专题国家天文台_光学天文研究部
作者单位Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Shi, Fei,Zhao, Gang,Wicker, James. Oxygen Abundance Methods in SDSS: View from Modern Statistics[J]. JOURNAL OF ASTROPHYSICS AND ASTRONOMY,2010,31(3):121-133.
APA Shi, Fei,Zhao, Gang,&Wicker, James.(2010).Oxygen Abundance Methods in SDSS: View from Modern Statistics.JOURNAL OF ASTROPHYSICS AND ASTRONOMY,31(3),121-133.
MLA Shi, Fei,et al."Oxygen Abundance Methods in SDSS: View from Modern Statistics".JOURNAL OF ASTROPHYSICS AND ASTRONOMY 31.3(2010):121-133.

入库方式: OAI收割

来源:国家天文台

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