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Extensive X-ray variability studies of NGC 7314 using long XMM-Newton observations

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journal contribution
posted on 17.11.2016, 11:46 by D. Emmanoulopoulos, I. M. McHardy, S. Vaughan, I. E. Papadakis
We present a detailed X-ray variability study of the low-mass active galactic nuclei (AGN) NGC 7314 using the two newly obtained XMM–Newton observations (140 and 130 ks), together with two archival data sets of shorter duration (45 and 84 ks). The relationship between the X-ray variability characteristics and other physical source properties (such as the black hole mass) are still relatively poorly defined, especially for low-mass AGN. We perform a new, fully analytical, power spectral density (PSD) model analysis method, which will be described in detail in a forthcoming paper, that takes into consideration the spectral distortions, caused by red-noise leak. We find that the PSD in the 0.5–10 keV energy range, can be represented by a bending power law with a bend around 6.7 × 10−5 Hz, having a slope of 0.51 and 1.99 below and above the bend, respectively. Adding our bend time-scale estimate, to an already published ensemble of estimates from several AGN, supports the idea that the bend time-scale depends linearly only on the black hole mass and not on the bolometric luminosity. Moreover, we find that as the energy range increases, the PSD normalization increases and there is a hint that simultaneously the high-frequency slope becomes steeper. Finally, the X-ray time-lag spectrum of NGC 7314 shows some very weak signatures of relativistic reflection, and the energy resolved time-lag spectrum, for frequencies around 3 × 10−4 Hz, shows no signatures of X-ray reverberation. We show that the previous claim about ks time delays in this source, is simply an artefact induced by the minuscule number of points entering during the time-lag estimation in the low-frequency part of the time-lag spectrum (i.e. below 10−4 Hz).

Funding

DE and IMM acknowledge the Science and Technology Facilities Council (STFC) for support under grant ST/G003084/1. SV acknowledges the STFC for support under grant ST/K001000/1. DE is grateful to Dr Abdu Zoghbi who provided all the necessary information about the analysis methods used in ZO13 during the workshop ‘The X-ray Spectral-Timing Revolution’ in 2016 February, Leiden, the Netherlands. This research has made use of NASA’s Astrophysics Data System Bibliographic Services.

History

Citation

Monthly Notices of the Royal Astronomical Society, 2016, 460 (3), pp. 2413-2431

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

VoR (Version of Record)

Published in

Monthly Notices of the Royal Astronomical Society

Publisher

Oxford University Press (OUP), Royal Astronomical Society

issn

0035-8711

eissn

1365-2966

Acceptance date

10/05/2016

Available date

17/11/2016

Publisher version

http://mnras.oxfordjournals.org/content/460/3/2413

Language

en