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Fig. 2


Light curves of TU UMa from different datasets: DA – DASCH A, DB – DASCH B, HIPP – Hipparcos, LIAKOS – Liakos & Niarchos (2011a, V, OUR – this paper (1-inch, green-filter), WASP – SuperWASP (CCD 144), PI – Pi of the Sky, NSVS – NSVS, MODEL – used template curves (DASCH templates are described in Sect. 3.4). Light curves are vertically shifted to better display the light variability.

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