11 Nov 2008 These are the webpages relative to Sherpa in the CIAO 3.4 release (18 December 2006). They are no longer actively updated, however the CXC will continue limited support of CIAO 3.4 for the near future. 15 Dec 2008 The newest version of the Chandra Interactive Analysis of Observations software, is CIAO 4.1, released on 15 December 2008. Read the release notes for detailed information. This release requires that CALDB 4.1.0 be installed for the software to work correctly. |
Sherpa Threads for CIAO 3.4When running a thread for the first time, you may wish to follow along, using the actual data employed in the thread. Please see the Getting Started thread for instructions on how to download and use the example data. All threadsA list of all the threads on one page. IntroductoryThese threads explain the basics of Sherpa: reading data, establishing models, fitting, and plotting. Information on how to customize plots via the Sherpa state objects (a.k.a. configuration variables) is covered as well. FittingSherpa provides extensive facilities for modeling and fitting data. The topics here range from basic fits using source spectra and responses to more advanced areas such as simultaneous fits to multiple datasets, accounting for the effects of pileup, and fitting spatial and grating data. PlottingSherpa allows the user to plot data, fits, statistics, ARFs, contours, surfaces, and more. These threads describe the basics of plotting as well as various methods for customizing plots. StatisticsSherpa provides numerous tools for determining goodness of fit, errors in parameter values, confidence intervals, and other statistical measures of a model's validity. These threads describe how to use these tools in your analysis. S-LangThe S-Lang language and Sherpa/S-Lang module provide a powerful means of extending Sherpa's capabilities through custom-made functions and scripts. The threads here introduce Sherpa's S-Lang functionality and provide some examples of its use. MiscellaneousThese threads describe other tasks that one can perform using Sherpa. DatasetsLinks to the datasets used in the threads. |
The Chandra X-Ray
Center (CXC) is operated for NASA by the Smithsonian Astrophysical Observatory. 60 Garden Street, Cambridge, MA 02138 USA. Email: cxcweb@head.cfa.harvard.edu Smithsonian Institution, Copyright © 1998-2004. All rights reserved. |