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CURious Variables Experiment (CURVE): CCD photometry of active dwarf nova DI Ursae Majoris

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Table 1 presents a journal of our CCD observations of DI UMa. In the following parts of this article (for convinience), civil dates are used to characterize moments of observations, rather than the corresponding HJD
Fig. 1. Global light curve of DI UMa during the 2007 campaign. Dots, plus signs and circles indicate di fferent periods of DI UMa activity
Fig. 4. Nightly light curves of DI UMa from its April 2007 superoutburst. Consecutive nights are denoted by dates in top-left /right corner
Fig. 6. Detrended light curve from data collected during all observed superoutbursts in 2007 campaign, folded with superhump period of P sh = 0.05504 days.
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