Temporal and spectral variability of PKS 0048−097 observed with Swift/XRT and Fermi/LAT. The following panels present the X-ray temporal and spectral variability and the γ-ray temporal and spectral variability. For Swift/XRT observations one point correspond to one day of observations, while in the case of Fermi/LAT data one point is for weekly integrated observations. We plot the flux upper limits in the Fermi/LAT light curve with grey points. The time periods corresponding to A and B flares are marked in grey, while the quiescence period Q is shown in blue.