We present the results of unfiltered and UBVR_cI_c band CCD photometry fast nova V2467Cyg. Our analysis of the data gives two distinct frequencies corresponding to periods of ~3.8h and ~35 min. The observed light curve of V2467 Cyg is typical for an intermediate polar.
@article{arxiv.0909.5149,
title = {V2467 Cygni as possible intermediate polar},
author = {E. Swierczynski and M. Mikolajewski and T. Tomov and E. Ragan and C. Galan and A. Karska and P. Wychudzki and M. Wiecek and M. Cikala and M. Lewandowski},
journal= {arXiv preprint arXiv:0909.5149},
year = {2010}
}