activity
19962023
most citedASCA observations of Seyfert 1 galaxies: II. Relativistic Iron K-alpha emission

592 citations · 9.1k across the 138 of their papers we have counts for

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8 papers · 1 filter

astro-ph.CO2013★ 35 cited

A High Resolution View of the Warm Absorber in the Quasar MR2251-178

J. N. Reeves, D. Porquet, V. Braito +5

High resolution X-ray spectroscopy of the warm absorber in the nearby quasar, MR2251-178 (z = 0.06398) is presented. The observations were carried out in 2011 using the Chandra Hig…

astro-ph.CO2012★ 41 cited

Modeling the Fe K Line Profiles in Type I AGN with a Compton-Thick Disk Wind

M. M. Tatum, T. J. Turner, S. A. Sim +4

We have modeled a small sample of Seyfert galaxies that were previously identified as having simple X-ray spectra with little intrinsic absorption. The sources in this sample all c…

astro-ph.CO2012★ 13 cited

Observations of Outflowing UV Absorbers in NGC 4051 with the Cosmic Origins Spectrograph

S. B. Kraemer, D. M. Crenshaw, J. P. Dunn +6

We present new Hubble Space Telescope (HST)/Cosmic Origins Spectrograph observations of the Narrow-Line Seyfert 1 galaxy NGC 4051. These data were obtained as part of a coordinated…

astro-ph.CO2011

X-ray Signatures of Circumnuclear Gas in AGN

T. J. Turner, L. Miller, M. Tatum

X-ray spectra of AGN are complex. X-ray absorption and emission features trace gas covering a wide range of column densities and ionization states. High resolution spectra show the…

astro-ph.CO2010★ 65 cited

A Multi-Wavelength Study of the Nature of Type 1.8/1.9 Seyfert Galaxies

M. L. Trippe, D. M. Crenshaw, R. P. Deo +4

We focus on determining the underlying physical cause of a Seyfert galaxy's appearance as type a 1.8 or 1.9. Are these "intermediate" Seyfert types typical Seyfert 1 nuclei with re…

astro-ph.CO2010★ 10 cited

Significant X-ray Line Emission in the 5-6 keV band of NGC 4051

T. J. Turner, L. Miller, J. N. Reeves +4

A Suzaku X-ray observation of NGC 4051 taken during 2005 Nov reveals line emission at 5.44 keV in the rest-frame of the galaxy which does not have an obvious origin in known rest-f…