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。
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.
出处
《广州大学学报(自然科学版)》
CAS
2011年第1期26-30,共5页
Journal of Guangzhou University:Natural Science Edition
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)
关键词
数据分析
吸收线
类星体
data analysis
absorption lines
quasars