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19932015
most citedAn XMM-Newton survey of broad iron lines in Seyfert galaxies

625 citations · 8.4k across the 88 of their papers we have counts for

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astro-ph2003★ 140 cited

The XMM-Newton Iron Line Profile of NGC 3783

J. N Reeves, K. Nandra, I. M. George +3

We report on observations of the iron K line in the nearby Seyfert 1 galaxy, NGC 3783, obtained in a long, 2 orbit (240 ks) XMM-Newton observation. The line profile obtained exhibi…

astro-ph2003★ 28 cited

A warm hot intergalactic medium towards 3C 120?

B. McKernan, T. Yaqoob, R. Mushotzky +2

We observed the Seyfert I active galaxy/broad line radio galaxy 3C120 with the Chandra high energy transmission gratings and present an analysis of the soft X-ray spectrum. We iden…

astro-ph2003★ 204 cited

The Ionized Gas and Nuclear Environment in NGC 3783. IV. Variability and Modeling of the 900 ks CHANDRA Spectrum

H. Netzer, S. Kaspi, E. Behar +12

We present a detailed spectral analysis of the data obtained from NGC 3783 during the period 2000-2001 using Chandra. This analysis leads us to the following results. 1) NGC 3783 f…

astro-ph2003★ 89 cited

Fe XXV and Fe XXVI Diagnostics of the Black Hole and Accretion Disk in Active Galaxies: Chandra Time-Resolved Spectroscopy of NGC 7314

T. Yaqoob, I. M. George, T. R. Kallman +3

We report the detection of Fe XXV and Fe XXVI emission lines from a Chandra HETGS observation of the Seyfert~1 galaxy NGC 7314, made simultaneously with RXTE. The lines are re…

astro-ph2003★ 51 cited

The Ionized Gas and Nuclear Environment in NGC 3783 III. Detection of a Decreasing Radial Velocity in an Intrinsic UV Absorber

J. R. Gabel, D. M. Crenshaw, S. B. Kraemer +14

We report an intrinsic absorber with decreasing outflow velocity in the Seyfert 1 galaxy NGC 3783. This is the first detection of a change in radial velocity in an outflow associat…

astro-ph2003

Elemental Abundances in NGC 3516

T. J. Turner, S. B. Kraemer, R. F. Mushotzky +2

We present RGS data from an XMM-Newton observation of the Seyfert 1 galaxy NGC 3516, taken while the continuum source was in an extreme low state. The spectrum shows numerous emiss…