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Fig. 7
The X-ray (2–10 keV) vs. the FIR (4–100 μm) relation for our sources. The solid and dotted lines denote the best-fit relation of Ranalli et al. (2003), and its associated 2σ error, for normal galaxies in the local Universe. Open circles denote the four sources classified as galaxies on the basis of the X-ray diagnostics.
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