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19992020
most citedThe Ultraluminous State

463 citations · 6.1k across the 68 of their papers we have counts for

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35 papers · 1 filter

astro-ph2008★ 55 cited

A Comprehensive X-ray Spectral Analysis of the Seyfert 1.5 NGC 3227

A. Markowitz, J. N. Reeves, I. M. George +5

We present results of a 100 ks XMM observation of the Seyfert 1.5 NGC 3227. Our best-fit broadband model to the pn spectrum consists of a moderately flat (photon index 1.57) hard X…

astro-ph2008★ 50 cited

On the evidence for narrow, relativistically shifted X-ray lines

S. Vaughan, P. Uttley

In recent years there have been many reported detections of highly redshifted or blueshifted narrow spectral lines (both emission or absorption) in the X-ray spectra of active gala…

astro-ph2008★ 45 cited

Line Searches in Swift X-ray Spectra

C. P. Hurkett, S. Vaughan, J. P. Osborne +14

Prior to the launch of the Swift mission several X-ray line detections were reported in Gamma Ray Burst afterglow spectra. To date, these pre-Swift era results have not been conclu…

astro-ph2008★ 2 cited

Studying accreting black holes and neutron stars with time series: beyond the power spectrum

S. Vaughan, P. Uttley

The fluctuating brightness of cosmic X-ray sources, particularly accreting black holes and neutron star systems, has enabled enormous progress in understanding the physics of turbu…

astro-ph2006★ 34 cited

X-ray reflection in the nearby Seyfert 2 galaxy NGC 1068

K. Pounds, S. Vaughan

We use the full broad-band XMM-Newton EPIC data to examine the X-ray spectrum of the nearby Seyfert 2 galaxy NGC 1068, previously shown to be complex with the X-ray continuum being…

astro-ph2005★ 335 cited

An origin for short g-ray bursts unassociated with current star formation

S. D. Barthelmy, G. Chincarini, D. N. Burrows +28

Two short (<2 s) g-ray bursts (GRBs) have recently been localized and fading afterglow counterparts detected. The combination of these two results left unclear the nature of the ho…

astro-ph2005★ 108 cited

Discovery of an Afterglow Extension of the Prompt Phase of Two Gamma Ray Bursts Observed by Swift

S. D. Barthelmy, J. K. Cannizzo, N. Gehrels +19

BAT and XRT observations of two recent well-covered GRBs observed by Swift, GRB 050315 and GRB 050319, show clearly a prompt component joining the onset of the afterglow emission.…

astro-ph2005★ 42 cited

The dust-scattered X-ray halo around Swift GRB 050724

S. Vaughan, R. Willingale, P. Romano +12

This paper discusses the X-ray halo around the Swift gamma-ray burst GRB 050724 (z=0.258), detected by the Swift X-Ray Telescope. The halo, which forms a ring around the fading X-r…

astro-ph2005★ 160 cited

Swift observations of the X-ray bright GRB 050315

S. Vaughan, M. R. Goad, A. P. Beardmore +30

This paper discusses Swift observations of the gamma-ray burst GRB 050315 (z=1.949) from 80 s to 10 days after the onset of the burst. The X-ray light curve displayed a steep early…

astro-ph2005★ 37 cited

The soft X-ray blast in the apparently sub-luminous GRB 031203

D. Watson, S. A. Vaughan, R. Willingale +11

GRB031203 was a very low apparent luminosity gamma-ray burst (GRB). It was also the first GRB with a dust-scattered X-ray halo. The observation of the halo allowed us to infer the…

astro-ph2005★ 30 cited

Detecting X-ray QPOs in Active Galaxies

S. Vaughan, P. Uttley

Since EXOSAT produced the first good quality X-ray light curves of Seyfert galaxies there have been several claims of quasi-periodic oscillations (QPOs). None of these have withsto…

astro-ph2005★ 65 cited

Where are the X-ray QPOs in active galaxies?

S. Vaughan, P. Uttley

In this paper we address the question of whether existing X-ray observations of Seyfert galaxies are sufficiently sensitive to detect quasi-periodic oscillations (QPOs) similar to…

astro-ph2004★ 4 cited

Rapid X-ray Variability of Seyfert 1 Galaxies

S. Vaughan, A. C. Fabian, K. Iwasawa

The rapid and seemingly random fluctuations in X-ray luminosity of Seyfert galaxies provided early support for the standard model in which Seyferts are powered by a supermassive bl…

astro-ph2004

The exceptional X-ray variability of the dwarf Seyfert nucleus NGC 4395

S. Vaughan, K. Iwasawa, A. C. Fabian +1

An analysis of the X-ray variability of the low luminosity Seyfert nucleus NGC 4395, based on a long XMM-Newton observation, is presented. The power spectrum shows a clear break fr…

astro-ph2004★ 5 cited

The narrow-line quasar NAB 0205+024 observed with XMM-Newton

L. C. Gallo, Th. Boller, W. N. Brandt +2

The XMM-Newton observation of the narrow-line quasar NAB 0205+024 reveals three striking differences since it was last observed in the X-rays with ASCA. Firstly, the 2-10 keV power…

astro-ph2004★ 170 cited

X-ray reflection in the NLS1 1H 0707-495

A. C. Fabian, G. Miniutti, L. Gallo +4

We apply a reflection-dominated model to the second XMM-Newton observation of the Narrow Line Seyfert 1 galaxy 1H 0707-495. As in the first XMM-Newton observation a sharp spectral…

astro-ph2004★ 71 cited

Long-term spectral changes in the partial-covering candidate NLS1 1H 0707-495

L. C. Gallo, Y. Tanaka, Th. Boller +3

We compare two XMM-Newton observations of the Narrow-Line Seyfert 1 galaxy 1H 0707-495 separated by two years, and discuss the results in terms of the partial-covering phenomenon.…

astro-ph2004★ 72 cited

An XMM-Newton observation of Ark 120: the X-ray spectrum of a `bare' Seyfert 1 nucleus

S. Vaughan, A. C. Fabian, D. R. Ballantyne +3

We report on a long (100 ks) XMM-Newton observation of the bright Seyfert 1 galaxy Arakelian 120. The source previously showed no signs of intrinsic reddening in its infrared-ultra…

astro-ph2004★ 32 cited

Chandra observations of five X-ray transient galactic nuclei

S. Vaughan, R. Edelson, R. S. Warwick

We report on exploratory Chandra observations of five galactic nuclei that were found to be X-ray bright during the ROSAT all-sky survey (with L_X > 10^43 erg s^-1) but subsequentl…

astro-ph2003★ 183 cited

A long, hard look at MCG-6-30-15 with XMM-Newton II: detailed EPIC analysis and modelling

S. Vaughan, A. C. Fabian

The bright Seyfert 1 galaxy MCG-6-30-15 has provided some of the best evidence to date for the existence of supermassive black holes in active galactic nuclei. Observations with AS…

astro-ph2003★ 21 cited

A long hard look at MCG-6-30-15 with XMM-Newton and BeppoSAX

S. Vaughan, A. C. Fabian, K. Iwasawa +1

We summarise the primary results from a 320 ks observation of the bright Seyfert 1 galaxy MCG-6-30-15 with XMM-Newton and Beppo-SAX.

astro-ph2003★ 74 cited

XMM-Newton spectral properties of the Narrow-Line Seyfert 1 galaxy IRAS 13224--3809

Th. Boller, Y. Tanaka, A. Fabian +5

We report on the first XMM-Newton observation of the highly X-ray variable, radio-quiet, Narrow-Line Seyfert 1 galaxy IRAS 13224-3809 obtained during the guaranteed time programme…

astro-ph2003★ 64 cited

A two-component ionized reflection model of MCG--6-30-15

D. R. Ballantyne, S. Vaughan, A. C. Fabian

Ionized reflection has often been considered as the explanation for the unusual Fe K variability observed in MCG--6-30-15. In this paper, we test this model using a 325 ks observat…

astro-ph2003★ 173 cited

The iron line in MCG-6-30-15 from XMM-Newton: evidence for gravitational light-bending?

A. C. Fabian, S. Vaughan

The lack of variability of the broad iron line seen in the Seyfert 1 galaxy MCG-6-30-15 is studied using the EPIC pn data obtained from a 2001 observation of 325 ks, during which t…