ON CALIBRATIONS USING THE CRAB NEBULA AND MODELS OF THE NEBULAR X-RAY EMISSION

被引:42
|
作者
Weisskopf, M. C. [1 ]
Guainazzi, M. [2 ]
Jahoda, K. [3 ]
Shaposhnikov, N. [4 ]
O'Dell, S. L. [1 ]
Zavlin, V. E. [5 ]
Wilson-Hodge, C. [1 ]
Elsner, R. F. [1 ]
机构
[1] NASA, MSFC, Space Sci Off, Huntsville, AL 35812 USA
[2] ESAC, Madrid, Spain
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] Univ Maryland, CRESST, GSFC, Dept Astron, College Pk, MD 20742 USA
[5] Space Sci Off, MSFC, USRA, Huntsville, AL 35812 USA
来源
ASTROPHYSICAL JOURNAL | 2010年 / 713卷 / 02期
关键词
instrumentation: miscellaneous; ISM: supernova remnants; methods: data analysis; pulsars: individual (Crab Pulsar); X-rays: individual (Crab Nebula); SPECTROSCOPY; PULSAR;
D O I
10.1088/0004-637X/713/2/912
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Motivated by a paper of Kirsch et al. on possible use of the Crab Nebula as a standard candle for calibrating X-ray response functions, we examine consequences of intrinsic departures from a single (absorbed) power law upon such calibrations. We limit our analyses to three more modern X-ray instruments-the ROSAT/PSPC, the RXTE/Proportional Counter Array, and the XMM-Newton/EPIC-pn (burst mode). The results indicate a need to refine two of the three response functions studied. We are also able to distinguish between two current theoretical models for the system spectrum.
引用
收藏
页码:912 / 919
页数:8
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