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We present and discuss BeppoSAX observations of Mrk841 and Mrk335, twoSeyfert 1 galaxies in which previous observations have established the presenceof soft excesses. We confirm the soft excess in both sources, even if forMrk~841 a warm absorber provides a fit almost as good as the one with a trueexcess. As far as the hard X-ray continuum is concerned, a Comptonization modelprovides a fit as good as a power law and a physically sound solution forMrk841. For Mrk335, the Comptonization model gives a result which is somewhatbetter on statistical ground, but rather problematic on physical ground. Themost interesting results regard the reprocessing components. For Mrk841 we finda very large reflection continuum but an almost normal iron line equivalentwidth even if, within the errors, a solution in which both components are afactor ~2 larger than expected for an accretion disc is still marginallyacceptable. If this is the case, an anisotropy of the primary emission seemsthe best explanation. On the contrary, in Mrk335 we find a very large iron lineEW but a reflection component not accordingly large. In this case, the bestsolution seems to be in terms of reflection from an ionized disc.Comment: Accepted for publication in A&

BeppoSAX observations of Mrk 841 and Mrk 335