activity
20032009
most citedA Compton-thick Wind in the High Luminosity Quasar, PDS 456

197 citations · 318 across the 4 of their papers we have counts for

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9 papers · 1 filter

astro-ph2008106 cited

Multi-dimensional modelling of X-ray spectra for AGN accretion-disk outflows

S. A. Sim, K. S. Long, L. Miller +1

We use a multi-dimensional Monte Carlo code to compute X-ray spectra for a variety of active galactic nucleus (AGN) disk-wind outflow geometries. We focus on the formation of blue-…

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-ph200772 cited

Spitzer/IRS Observations of Seyfert 1.8s and 1.9s: A Comparison with Seyfert 1s and Seyfert 2s

R. P. Deo, D. M. Crenshaw, S. B. Kraemer +4

We present Spitzer Space Telescope mid-infrared spectra of 12 Seyfert 1.8 and 1.9 galaxies over the 5-38 um region. We compare the spectral characteristics of this sample to those…

astro-ph200770 cited

Low accretion rates at the AGN cosmic downsizing epoch

A. Babic, L. Miller, M. J. Jarvis +3

Context: X-ray surveys of Active Galactic Nuclei (AGN) indicate `cosmic downsizing', with the comoving number density of high-luminosity objects peaking at higher redshifts (z abou…

astro-ph200777 cited

The Variable X-ray Spectrum of Markarian 766 - II. Time-Resolved Spectroscopy

T. J. Turner, L. Miller, J. N. Reeves +1

CONTEXT: The variable X-ray spectra of AGN systematically show steep power-law high states and hard-spectrum low states. The hard low state has previously been found to be a compon…

astro-ph2006109 cited

The variable X-ray spectrum of Markarian 766 - I. Principal components analysis

L. Miller, T. J. Turner, J. N. Reeves +3

Aims: We analyse a long XMM-Newton spectrum of the narrow-line Seyfert 1 galaxy Mrk 766, using the marked spectral variability on timescales >20ks to separate components in the X-r…