Additional funding was provided by the JWST Mission office at Space Telescope Science Institute to improve capabilities for 3-D data visualization. SAOImage DS9 development has been made possible by funding from the Chandra X-ray Science Center (CXC) and the High Energy Astrophysics Science Archive Center (HEASARC). GUI elements such as the coordinate display, panner, magnifier, horizontal and vertical graphs, button bar, and color bar can be configured via menus or the command line. Most of this software is designed for professional researchers and advanced students for the analysis of scientific astronomical observations in FITS format. For the final data analysis, any plotting/fitting tool (e.g. HEASARC Software The following software is supported by the HEASARC. All versions and platforms support a consistent set of GUI and functional capabilities.ĭS9 supports advanced features such as 2-D, 3-D and RGB frame buffers, mosaic images, tiling, blinking, geometric markers, colormap manipulation, scaling, arbitrary zoom, cropping, rotation, pan, and a variety of coordinate systems. Images can be displayed with the viewer SAOIMAGE DS9 or Pythons matplotlib package. It requires no installation or support files. It provides for easy communication with external analysis tasks and is highly configurable and extensible via XPA and SAMP.ĭS9 is a stand-alone application. Smithsonian Astrophysical Observatory Image DS9 (SAOImage DS9) is an astronomical imaging and data visualization application. ![]() DS9 supports FITS images and binary tables, multiple frame buffers, region manipulation, and many scale algorithms and colormaps. provides for easy communication with external analysis tasks and is highly configurable and extensible via XPA and SAMP.DS9 is a stand. SAOImage DS9 is an astronomical imaging and data visualization application, compatible with FITS files. ![]() SAOImage DS9 is an astronomical imaging and data visualization application. SAOImage DS9 is an astronomical imaging and data visualization application. DS9 supports FITS images and binary tables, multiple frame buffers, region manipulation, and many scale algorithms and colormaps.
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