Fitting models to spectra with small numbers of counts/bin.
Abstract
Many Chandra and XMM spectra have small numbers of counts per resolution element. I will discuss different approaches to fitting models to these spectra using XSPEC.
- Publication:
-
AAS/High Energy Astrophysics Division #5
- Pub Date:
- October 2000
- Bibcode:
- 2000HEAD....5.1003A