Hardness ratio estimation in low counting X-ray photometry

被引:10
作者
Jin, Y. K. [1 ]
Zhang, S. N.
Wu, J. F.
机构
[1] Tsing Hua Univ, Dept Engn Phys, Beijing 100084, Peoples R China
[2] Tsing Hua Univ, Ctr Astrophys, Beijing 100084, Peoples R China
[3] Tsing Hua Univ, Dept Phys, Beijing 100084, Peoples R China
[4] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
关键词
methods : statistical; X-rays : general; X-rays : ISM;
D O I
10.1086/508677
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Hardness ratios are commonly used in X-ray photometry to roughly indicate spectral properties. They are usually defined as the ratio of counts in two different wave bands. This definition, however, is problematic when the counts are very limited. Here we instead define the hardness ratio using the lambda-parameter of Poisson processes and develop an estimation method via Bayesian statistics. Our Monte Carlo simulations show the validity of our method. Based on this new definition we can estimate the hydrogen column density for the photoelectric absorption of X-ray spectra in the case of low counting statistics.
引用
收藏
页码:1566 / 1570
页数:5
相关论文
共 9 条
[2]   ERRORS ON RATIOS OF SMALL NUMBERS OF EVENTS [J].
JAMES, F ;
ROOS, M .
NUCLEAR PHYSICS B, 1980, 172 (2-3) :475-480
[3]   The selection of prior distributions by formal rules [J].
Kass, RE ;
Wasserman, L .
JOURNAL OF THE AMERICAN STATISTICAL ASSOCIATION, 1996, 91 (435) :1343-1370
[4]   Bayesian estimation of hardness ratios: Modeling and computations [J].
Park, Taeyoung ;
Kashyap, Vinay L. ;
Siemiginowska, Aneta ;
Van Dyk, David A. ;
Zezas, Andreas ;
Heinke, Craig ;
Wargelin, Bradford J. .
ASTROPHYSICAL JOURNAL, 2006, 652 (01) :610-628
[5]  
PROSPER HB, 1985, NUCL INSTRUM METH A, V241, P236, DOI 10.1016/0168-9002(85)90539-X
[6]   Chandra observations of diffuse gas and luminous X-ray sources around the X-ray-bright elliptical galaxy NGC 1600 [J].
Sivakoff, GR ;
Sarazin, CL ;
Carlin, JL .
ASTROPHYSICAL JOURNAL, 2004, 617 (01) :262-280
[7]  
TENNANT AF, 2001, APJ, V549, P43
[8]   Analysis of energy spectra with low photon counts via Bayesian posterior simulation [J].
Van Dyk, DA ;
Connors, A ;
Kashyap, VL ;
Siemiginowska, A .
ASTROPHYSICAL JOURNAL, 2001, 548 (01) :224-243
[9]  
WU JF, 2006, IN PRESS CHINESE J A