activity
20032008
most citedDiscovery of multiple Lorentzian components in the X-ray timing properties of the Narrow Line Seyfert 1 Ark 564

160 citations · 395 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph200865 cited

X-ray Variability of the Seyfert 1 Markarian 335: Power Spectrum and Time Lags

P. Arevalo, I. M. McHardy, D. P. Summons

To investigate further the comparison between AGN and black hole X-ray binaries, we have studied the main X-ray variability properties of the Seyfert 1 Galaxy Markarian 335. We put…

astro-ph200817 cited

Fourier-resolved energy spectra of the Narrow Line Seyfert 1 Mkn 766

P. Arevalo, I. M. McHardy, A. Markowitz +4

We compute Fourier-resolved X-ray spectra of the Seyfert 1 Markarian 766 to study the shape of the variable components contributing to the 0.3-10 keV energy spectrum and their time…

astro-ph2007160 cited

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

I. M. McHardy, P. Arevalo, P. Uttley +4

We present a power spectral analysis of a 100 ksec XMM-Newton observation of the narrow line Seyfert 1 galaxy Ark~564. When combined with earlier RXTE and ASCA observations, these…

astro-ph200731 cited

Timing evidence in determining the accretion state of the Seyfert galaxy NGC 3783

D. P. Summons, P. Arevalo, I. M. McHardy +2

Previous observations with the Rossi X-ray Timing Explorer (RXTE) have suggested that the power spectral density (PSD) of NGC 3783 flattens to a slope near zero at low frequencies,…

astro-ph200655 cited

The Energy-dependent X-ray Timing Characteristics of the Narrow Line Seyfert 1 Mkn 766

A. Markowitz, I. E. Papadakis, P. Arevalo +3

We present the energy-dependent power spectral density (PSD) and cross-spectral properties of Mkn 766, obtained from combining data obtained during an XMM-Newton observation spanni…

astro-ph200667 cited

Spectral-timing evidence for a Very High State in the Narrow Line Seyfert 1 Ark 564

P. Arevalo, I. E. Papadakis, P. Uttley +2

We use a 100 ks long XMM-Newton observation of the Narrow-Line Seyfert 1 galaxy Ark 564 and combine it with the month-long monitoring of the same source produced by ASCA, to calcul…