2025MNRAS.544.3260L

Accreting supermassive black holes at the centres of galaxies are the engine of active galactic nuclei (AGNs). X-ray light curves of unabsorbed AGNs show dramatic random variability on time-scales ranging from seconds to years. The power spectrum of the fluctuations is usually well modelled with a power law that decays as $1/f$ at low frequencies, and which bends to $1/f^{2-3}$ at high frequencies. The time-scale associated with the bend correlates well with the mass of the black hole and may also correlate with bolometric luminosity in the 'X-ray variability plane'. Because AGN light curves are usually irregularly sampled, the estimation of AGN power spectra is challenging. In a previous paper, we introduced a new method to estimate the parameters of bending power law power spectra from AGN light curves. We apply this method to a sample of 56 variable and unabsorbed AGNs, observed with XMM-Newton and Swift in the 0.3-1.5 keV band over the past two decades. We obtain estimates of the bends in 50 sources, which is the largest sample of X-ray bends in the soft band. We also find that the high-frequency power spectrum is often steeper than 2. We update the X-ray variability plane with new bend time-scale measurements spanning from 7 min to 62 d. We report the detections of low-frequency bends in the power spectra of five AGN, three of which are previously unpublished: 1H 1934-063, Mkn 766 and Mkn 279.