Multivariate Monte Carlo Methods for the Reflection Grating Spectrometers on XMM-Newton
arXiv:astro-ph/0410644 · doi:10.1086/424436
Abstract
We propose a novel multivariate Monte Carlo method as an efficient and flexible approach to analyzing extended X-ray sources with the Reflection Grating Spectrometer (RGS) on XMM Newton. A multi-dimensional interpolation method is used to efficiently calculate the response function for the RGS in conjunction with an arbitrary spatially-varying spectral model. Several methods of event comparison that effectively compare the multivariate RGS data are discussed. The use of a multi-dimensional instrument Monte Carlo also creates many opportunities for the use of complex astrophysical Monte Carlo calculations in diffuse X-ray spectroscopy. The methods presented here could be generalized to other X-ray instruments as well.
36 pages, 14 figures, Accepted for publication in ApJ
References in corpus (7)
- High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies
- X-ray Imaging Spectroscopy of Abell 1835
- Chandra X-Ray Observatory (CXO):Overview
- XMM-Newton observations of the cluster of galaxies Sersic 159-03
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