Fig. 5

Differential I magnitudes of EE Cep obtained at Piwnice
Observatory during the 13 years from 1996 to 2010. The zero value corresponds to the
level of the average brightness outside (phases 0.4–0.8) eclipses. Below
+01 (i.e.
for magnitude changes smaller than +0
1) an
artificial, strongly non-linear scale is used to reduce the contrast in the
amplitude of the changes during and outside eclipses (thus, the relatively small
variations outside the eclipses can be seen and compared with the depth of the
eclipses).
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