activity
19982003
collaborators

7 papers

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-ph2002

The XMM-Newton view of the Galactic Centre

Masaaki Sakano, Robert S. Warwick, Anne Decourchelle

In X-rays, the Galactic Centre (GC) Region appears as a complex of diffuse thermal and non-thermal X-ray emission intermixed with a population of luminous discrete sources. Here we…

astro-ph2002

A new look at the X-ray properties of the Galaxy

R. S. Warwick

Observational programmes currently underway with both Chandra and XMM-Newton are set to revolutionize our view of our own Galaxy. This is fortunate since the X-ray band can provide…

astro-ph2002

The Galactic Plane Observed by XMM-Newton

A. Hands, R. Warwick, M. Watson +1

In A0-1 we proposed an ambitious long-term survey of selected regions of our Galaxy (the XGPS survey) using the EPIC CCD cameras on XMM-Newton. The first phase of the programme, wh…

astro-ph2002

The nature of ultraluminous X-ray sources in nearby galaxies

T. P. Roberts, M. R. Goad, M. J. Ward +2

The advanced capabilities of the Chandra and XMM-Newton observatories mean that, for the first time, the detailed study of the brightest point-like X-ray sources in nearby galaxies…

astro-ph1999

Evidence for an ionised disc in the narrow-line Seyfert 1 galaxy Ark 564

S. Vaughan, K. A. Pounds, J. Reeves +2

We present simultaneous ASCA and RXTE observations of Ark 564, the brightest known ``narrow-line'' Seyfert 1 in the 2-10 keV band. The measured X-ray spectrum is dominated by a ste…