Gamma-ray and optical oscillations in the blazar PKS 0537-441

We have considered the $\mathit{\text{Fermi}}$ $\gamma$-ray light curve of the blazar PKS 0537-441 during a high state extending from 2008/08/10 to 2011/08/27. The periodogram exhibits a peak at T $\sim$ 280 d, with a significance of $\sim$ 99.7 %. A peak of similar relevance at $\frac{1}{2}$ T is found in the optical light curves. Considering the entire duration of the $\mathit{\text{Fermi}}$ light curve 2008-2015, no significant peak is revealed, while the optical one remains meaningful. Comparing with recent observations of PKS 2155-304 and PG 1553+113 it seems that month-year oscillations can characterize some blazars. Month-scale oscillations can also show up only during phases of enhanced or bursting emission like in the case of PKS 0537-441.