A quasi-periodic modulation of the radio light curve of the blazar PKSB0048-097

In this letter we present the results of a wavelet analysis of the radio light curve of the BL Lac Object PKSB0048-097 from the University of Michigan Radio Astronomy Observatory monitoring program at 8 GHz during twenty-five years, from 1979 to 2004. The results show a remarkable periodicity of 450-470 days in the early 1980s that changed to a similar to 585 day periodicity in the late 1980s to early 1990s. A less pronounced similar to 400 day periodicity is found after similar to 1995. Very-long-baseline interferometry imaging at 15 GHz shows dramatic structural changes in the usually unresolved source between two epochs, 1995.57 and 2002.38. The pronounced northward directed jet seen in the 2002 image differs by more than 90 degrees in direction from the source structure found in earlier epochs. These findings make PKS B0048-097 a primary target for multi-wavelength observations and intensive radio monitoring to decipher the blazar-variability phenomenon.