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证认类星体吸收线方法（英文）
  • ISSN号：1000-8349
  • 期刊名称：《天文学进展》
  • 时间：0
  • 分类：P14[天文地球—天体物理;天文地球—天文学]
  • 作者机构：[1]广州大学天体物理中心,广东广州510006
  • 相关基金：Supported by National Natural Science Foundation of China（11073007 10573005 10273019）; National Natural Science Foundation of China（NSFC 10633010）; the 973 programme（2007CB815405）; the Bureau of Education of Guangzhou Municipality（11 Sui-Jiao-Ke[2009]）; GDUPS（2009）
作者： 覃一平[1], 陈志福[1]
关键词： 数据分析, 吸收线, 类星体, data analysis, absorption lines, quasars
中文摘要：

提出和完善了一个分析类星体能谱数据的方法.利用该方法,可以发现并测出类星体的吸收线.文章还通过取自Sloan Digital Sky Survey样本的3个类星体的能谱数据,演示了采用该方法证认MgII吸收线的结果

英文摘要：

We develop a method of analyzing the spectral data from quasar surveys.With this method,one can detect and measure absorption lines of quasars.The method is described in detail in this paper.In addition,we illustrate the method by identifying MgII absorption lines from the data of three quasars taken from the Sloan Digital Sky Survey.

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期刊信息
  • 《天文学进展》
  • 中国科技核心期刊
  • 主管单位:中国科学院
  • 主办单位:中国科学院上海天文台 中国天文学会
  • 主编：沈志强
  • 地址：上海市南丹路80号406
  • 邮编：200030
  • 邮箱：twxjz@shao.ac.cn
  • 电话：021-34775108
  • 国际标准刊号：ISSN：1000-8349
  • 国内统一刊号：ISSN：31-1340/P
  • 邮发代号:4-819
  • 获奖情况:
  • 1996年在第2届上海市优秀科技期刊评比中获得3等奖...,获得2011年上海市新闻出版局组织的期刊审读优秀奖
  • 国内外数据库收录:
  • 日本日本科学技术振兴机构数据库,中国中国科技核心期刊,中国北大核心期刊（2004版）,中国北大核心期刊（2008版）,中国北大核心期刊（2011版）,中国北大核心期刊（2014版）,中国北大核心期刊（2000版）
  • 被引量:1404