No CrossRef data available.
Article contents
Simulating Chandra observations of galaxy clusters
Published online by Cambridge University Press: 06 October 2004
Abstract
The direct comparison of observations to numerical hydro-N-body simulations, although simple in principle, is not always trivial because of possible artificial effects produced by the instrument response and by instrumental and sky background. To overcome this problem we build the software package X-MAS (X-ray MAp Simulator) devoted to simulate X-ray observations of galaxy clusters obtained from hydro-N-body simulations.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC195 , March 2004 , pp. 313 - 315
- Copyright
- © 2004 International Astronomical Union