On Calibrations using the Crab Nebula and Models of the Nebular X-ray Emission
arXiv:1003.1916 · doi:10.1088/0004-637X/713/2/912
Abstract
Motivated by a paper (Kirsch et al. 2005) 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/PCA, 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.
22 pages, 9 figures, accepted for publication in ApJ.
References in corpus (3)
- Non-thermal emission from relativistic MHD simulations of PWNe: from synchrotron to inverse Compton
- Effective area calibration of the Reflection Grating Spectrometers of XMM-Newton. I. X-ray spectroscopy of the Crab nebula
- The Subaru/XMM-Newton Deep Survey (SXDS) - VI. Properties of Active Galactic Nuclei Selected by Optical Variability
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