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X-ray time lags in PG 1211+143

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Abstract

We investigate the X-ray time lags of a recent ~630 ks XMM-Newton observation of PG 1211+143. We find well-correlated variations across the XMM-Newton EPIC bandpass, with the first detection of a hard lag in this source with a mean time delay of up to ~3 ks at the lowest frequencies. We find that the energy-dependence of the low-frequency hard lag scales approximately linearly with log(E) when averaged over all orbits, consistent with the propagating fluctuations model. However, we find that the low-frequency lag behaviour becomes more complex on timescales longer than a single orbit, suggestive of additional modes of variability. We also detect a high-frequency soft lag at ~10-4 Hz with the magnitude of the delay peaking at ? 0.8 ks, consistent with previous observations, which we discuss in terms of small-scale reverberation.

Acceptance Date Jan 15, 2018
Publication Date May 1, 2018
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Publisher Oxford University Press
Pages 225-234
DOI https://doi.org/10.1093/mnras/sty123
Keywords accretion, accretion discs, galaxies, active galaxies, individual, PG 1211+143, Seyfert, X-rays
Publisher URL https://doi.org/10.1093/mnras/sty123

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