Fig. 15.
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An application of the mkacispback tool for the supernova remnant G359.1−0.5. Left panel: 0.7–5.0 keV image of the G359.1−0.5 region. The source region, which covers all the four ACIS-I CCDs, is shown with the green ellipse. Right panel: extracted spectrum and the output spectral model of mkacispback, as well as their residuals, are shown. The residuals below ∼7 keV are large because a model for the source emission has not been included here.
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