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CCD UBVRI photometry is presented for type II SN 2004dj for about 1200 days,starting day 2 past discovery. The photometric behaviour is typical for SNeII-P, although some minor peculiarities are noticed. We compare the photometricdata for the host cluster S96 before and after SN 2004dj outburst and do notfind any significant changes.

Photometric investigation of bright type II-P Supernova 2004dj