Welcome to Sherpa’s documentation¶
Welcome to the Sherpa documentation. Sherpa is a Python package for modeling and fitting data. It was originally developed by the Chandra X-ray Center for use in analysing X-ray data (both spectral and imaging) from the Chandra X-ray telescope, but it is designed to be a general-purpose package, which can be enhanced with domain-specific tasks (such as X-ray Astronomy). Sherpa contains an expressive and powerful modeling language, coupled with a range of statistics and robust optimisers.
Sherpa is released under the GNU General Public License v3.0, and is compatible with Python versions 3.5, 3.6, and 3.7. It is expected that it will work with Python 3.8 but testing has been limited. Information on recent releases and citation information for Sherpa is available using the Digital Object Identifier (DOI) 10.5281/zenodo.593753.
The last version of Sherpa compatible with Python 2.7 was the 4.11.1 release.
- A quick guide to modeling and fitting in Sherpa
- Sherpa and CIAO
- What data is to be fit?
- Creating model instances
- Evaluating a model
- Available Models
- What statistic is to be used?
- Optimisers: How to improve the current parameter values
- Fitting the data
- Markov Chain Monte Carlo and Poisson data
- Utility routines
- Simple Interpolation
- Simple user model
At present there is no developer mailing list for Sherpa.