The X-ray properties of the PG QSO sample observed with XMM-Newton

被引：0
|
作者：
Jiménez, E [1 ]
Piconcelli, E [1 ]
Guainazzi, M [1 ]
Schartel, N [1 ]
机构：
[1] ESA, RSSD, Newton Sci Operat Ctr, XMM, E-28080 Madrid, Spain
来源：
MULTIWAVELENGTH AGN SURVEYS | 2004年
关键词：
D O I：
10.1142/9789812702432_0074
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present preliminary results of a systematic analysis of the XMM-Newton spectra of nearby optically bright QSOs. The objects have been selected from the Bright Quasar Survey sample. The goal of this project is to characterise the X-ray spectral properties of optically selected QSOs in the 0.3-12 keV energy band. In most cases, two component continua are sufficient to model reasonably well the observed spectra. All but one detected Fe K alpha line have narrow profiles.
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收藏
页码：307 / 308
页数：2
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