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Fig. 5
ASCA SIS spectra and residuals of NGC 7314 in the 1994 (left panel) and 1996 (right panel) observations. The solid line represents the power-law best-fit model to both SIS and GIS spectra excluding intrinsic absorption and the Fe Kα emission line. For clarity only the SIS0 and SIS1 spectra of each observation are plotted.
This figure is made of several images, please see below:
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