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20022009
most citedDiscovery of multiple Lorentzian components in the X-ray timing properties of the Narrow Line Seyfert 1 Ark 564

160 citations · 433 across the 13 of their papers we have counts for

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astro-ph2003

SAX J1808.4-3658 and the origin of X-ray variability in X-ray binaries and active galactic nuclei

Philip Uttley

The aperiodic X-ray variability in neutron star and black hole X-ray binaries (XRBs), and active galactic nuclei (AGN) shows a characteristic linear relationship between rms amplit…

astro-ph2003

Combined Long and Short Timescale X-ray Variability of NGC4051 with RXTE and XMM-Newton

I. M. McHardy, I. E. Papadakis, P. Uttley +2

We present over 6.5 years of frequent X-ray observations of the NLS1 galaxy NGC4051 by RXTE together with a >100ks observation by XMM-Newton and so derive a 2-10 keV PSD covering a…

astro-ph2003

Complex X-ray spectral behaviour of NGC 4051 in the low flux state

P. Uttley, R. D. Taylor, I. M. McHardy +4

The Narrow Line Seyfert 1 galaxy NGC 4051 was observed in one of its prolonged low-lux states by XMM-Newton in November 2002. Here we present the results of an analysis of EPIC-pn…

astro-ph2003

Catching NGC4051 in the low state with XMM-Newton

P. Uttley, R. D. Taylor, I. M. McHardy +4

The Narrow Line Seyfert 1 galaxy NGC4051 shows unusual low flux states, lasting several months, when the 2-10 keV X-ray spectrum becomes unusually hard (photon index<1) while the s…

astro-ph2003

Constraints on AGN accretion disc viscosity derived from continuum variability

Rhaana L. C. Starling, Aneta Siemiginowska, Phil Uttley +1

We estimate a value of the viscosity parameter in AGN accretion discs for the PG quasar sample. We assume that optical variability on time-scales of months to years is caused by lo…

astro-ph2003

Combined Long and Short Timescale X-ray Variability of NGC4051 with RXTE and XMM-Newton

I. M. McHardy, I. E. Papadakis, P. Uttley +2

We present a comprehensive examination of the X-ray variability of the narrow line Seyfert 1 (NLS1) galaxy NGC4051. We combine over 6.5 years of frequent monitoring observations by…