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most citedOn characterising the variability properties of X-ray light curves from active galaxies

1.2k citations · 6.7k across the 86 of their papers we have counts for

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astro-ph2003★ 56 cited

XMM-Newton observations of Sagittarius A East

Masaaki Sakano, Robert S. Warwick, Anne Decourchelle +1

We present an analysis of a recent XMM-Newton observation of Sgr A East, a supernova remnant located close to the Galactic Centre. Very high quality X-ray spectra reveal many emiss…

astro-ph2003★ 32 cited

An XMM-Newton view of M101: I. The luminous X-ray source population

L. P. Jenkins, T. P. Roberts, R. S. Warwick +2

We present the first results of an XMM-Newton EPIC observation of the luminous X-ray source population in the supergiant spiral galaxy M101. We have studied the properties of the f…

astro-ph2003

A new population of X-ray transients in the Galactic Centre

Masaaki Sakano, Robert S. Warwick, Anne Decourchelle +1

A comparison of the XMM-Newton and Chandra Galactic Centre (GC) Surveys has revealed two faint X-ray transients with contrasting properties. The X-ray spectrum of XMM J174544-2913.…

astro-ph2003★ 1 cited

Sgr A East and its surroundings observed in X-rays

Masaaki Sakano, Robert S. Warwick, Anne Decourchelle

We report the results of an XMM-Newton observation of Sgr A East and its surroundings. The X-ray spectrum of Sgr A East is well represented with a two-temperature plasma model with…

astro-ph2003★ 1.2k cited

On characterising the variability properties of X-ray light curves from active galaxies

S. Vaughan, R. Edelson, R. S. Warwick +1

We review some practical aspects of measuring the amplitude of variability in `red noise' light curves typical of those from Active Galactic Nuclei (AGN). The quantities commonly u…

astro-ph2003★ 216 cited

XMM-Newton observation of the brightest X-ray flare detected so far from SgrA*

D. Porquet, P. Predehl, B. Aschenbach +5

We report the high S/N observation on October 3, 2002 with XMM-Newton of the brightest X-ray flare detected so far from SgrA* with a duration shorter than one hour (~ 2.7 ks). The…