Fig. 2
Profiles of the relativistically broadened iron lines detected in the GREDOS sample. They represent ratios of the data to the model once the kyrline component is removed from the best-fit model. The lines in MCG-5-23-16 and NGC 5506 are detected at a confidence level ≥ 5σ in the relativistically blurred line scenario. The line in NGC 4507 is detected at a confidence level ≃ 3σ only.
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