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This paper is concerned with the regularity of solutions to parabolic
evolution equations. Special attention is paid to the smoothness in the
specific anisotropic scale $\ B^{r}_{\tau,\tau},
\frac{1}{\tau}=\frac{r}{d}+\frac{1}{p}\ $
measures the anisotropy. The regularity in these spaces determines the
approximation order that can be achieved by fully space-time adaptive
approximation schemes. In particular, we show that for the heat equation our
results significantly improve previous results by Aimar and Gomez [3].

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