Lobban, A. P.Turner, T. J.Reeves, J. N.Braito, V.Miller, L.2020-10-212020-10-212020-04-16Lobban, A. P.; Turner, T. J.; Reeves, J. N.; Braito, V.; Miller, L.; X-ray variability analysis of a large series of XMM–Newton +NuSTAR observations of NGC 3227; Monthly Notices of the Royal Astronomical Society, Volume 494, Issue 4, June 2020, Pages 5056–5074; https://academic.oup.com/mnras/article-abstract/494/4/5056/5820815?https://doi.org/10.1093/mnras/staa1008http://hdl.handle.net/11603/19945We present a series of X-ray variability results from a long XMM–Newton + NuSTAR campaign on the bright, variable AGN NGC 3227. We present an analysis of the light curves, showing that the source displays typically softer-when-brighter behaviour, although also undergoes significant spectral hardening during one observation which we interpret as due to an occultation event by a cloud of absorbing gas. We spectrally decompose the data and show that the bulk of the variability is continuum-driven and, through rms variability analysis, strongly enhanced in the soft band. We show that the source largely conforms to linear rms-flux behaviour and we compute X-ray power spectra, detecting moderate evidence for a bend in the power spectrum, consistent with existing scaling relations. Additionally, we compute X-ray Fourier time lags using both the XMM–Newton and – through maximum-likelihood methods – NuSTAR data, revealing a strong low-frequency hard lag and evidence for a soft lag at higher frequencies, which we discuss in terms of reverberation models.19 pagesen-USThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.This article is published in Monthly Notices of the Royal Astronomical Society ©: 2020 The Author(s), Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.Text