The complementarity between Chiral Perturbation Theory and the Linear Sigma Model is exploited to study production in radiative decays, where the effects of the scalar resonance, and those of its more controversial partner, should become manifest via the $\phi\to K^+ K^- (\gamma)\to\pi^0\pi^0\gamma $ decay chain. The recently reported data on coming from the VEPP-2M collider in Novosibirsk and the DANE -factory in Frascati can be reasonably described in our approach, which we propose as a promising first step towards more detailed analyses. The contribution, which appears as a moderately narrow peak at the high part of the dipion mass spectrum, can be interpreted as the isoscalar member of the scalar nonet with a large $f_0 K\bar{K}f_0\pi\pi\sigmaf_0$ mixing. Indeed, the mixing angle in the flavour basis is found to be , if the -propagator is approximated by a simple Breit-Wigner, or , if an improved two-channel analysis is performed. The resonance, which is then strongly coupled to pion pairs, yields a tiny contribution because, in our approach, its coupling to kaon pairs is proportional to and thus quite small.

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