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As part of a long term monitoring campaign of Mrk 335, deep XMM-Newtonobservations catch the narrow-line Seyfert 1 galaxy (NLS1) in a complex,intermediate flux interval as the active galaxy is transiting from low- tohigh-flux. Other works on these same data examined the general behaviour of theNLS1 (Grupe et al.) and the conditions of its warm absorber (Longinotti etal.). The analysis presented here demonstrates the X-ray continuum and timingproperties can be described in a self-consistent manner adopting a blurredreflection model with no need to invoke partial covering. The rapid spectralvariability appears to be driven by changes in the shape of the primary emitterthat is illuminating the inner accretion disc around a rapidly spinning blackhole (a > 0.7). While light bending is certainly prominent, the rather constantemissivity profile and break radius obtained in our spectral fitting suggestthat the blurring parameters are not changing as would be expected if theprimary source is varying its distance from the disc. Instead changes could beintrinsic to the power law component. One possibility is that material in anunresolved jet above the disc falls to combine with material at the base of thejet producing the changes in the primary emitter (spectral slope and flux)without changing its distance from the disc.

A blurred reflection interpretation for the intermediate flux state in Mrk 335