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The bright Narrow Emission Line Galaxy, NGC 5506, has been observedsimultaneously by XMM-Newton and BeppoSAX. The iron line is complex, with atleast two components: one narrow and corresponding to neutral iron, the secondone broad and corresponding to ionized iron. The latter line is equally wellfitted by a truly broad line or by a blend of He- and H-like narrow lines. Thebulk of the Compton reflection continuum originates in neutral matter, and istherefore associated with the narrow line: they are most likely emitted indistant matter. The origin of the ionized line(s) is less certain, but thesolution in terms of a blend of narrow lines from photoionized matter seems tobe preferable to emission from an ionized, relativistic accretion disc.Comment: accepted for publication in A&A Letter

The complex iron line of NGC 5506