collaborators

9 papers

astro-ph200820 cited

New XMM-Newton analysis of three bright X-ray sources in M31 globular clusters, including a new black hole candidate

R. Barnard, H. Stiele, D. Hatzidimitriou +6

We present detailed analysis of three globular cluster X-ray sources in the XMM-Newton extended survey of M31. The X-ray counterpart to the M31 globular cluster Bo 45 (XBo 45) was…

astro-ph200816 cited

An X-ray spectral survey of the disc of M31 with XMM-Newton

L. Shaw Greening, R. Barnard, U. Kolb +2

We present the results of a complete spectral survey of the X-ray point sources detected in five XMM-Newton observations along the major axis of M31 but avoiding the central bulge,…

astro-ph20088 cited

A multi-coloured survey of NGC 253 with XMM-Newton: testing the methods used for creating luminosity functions from low-count data

R. Barnard, L. Shaw Greening, U. Kolb

NGC 253 is a local, star-bursting spiral galaxy with strong X-ray emission from hot gas, as well as many point sources. We have conducted a spectral survey of the X-ray population…

astro-ph2007

A Multi-coloured survey of NGC 253 with XMM-Newton

R. Barnard, L. Shaw Greening, U. Kolb

There is a large body of work that has used the excellent Chandra observations of nearby galaxies with neglible low mass X-ray binary (LMXB) populations. This has culminated in a `…

astro-ph200722 cited

On the artificial nature of aperiodic variability in XMM-Newton observations of M31 X-ray sources and the ultraluminous X-ray source NGC 4559 ULX-7

R. Barnard, S. Trudolyubov, U. C. Kolb +3

Context: Power density spectra (PDS) that are characteristic of low mass X-ray binaries (LMXBs) have been previously reported for M31 X-ray sources, observed by XMM-Newton. However…

astro-ph2005

Cumulative luminosity functions of the X-ray point source population in M31

L. Shaw Greening, C. Tonkin, R. Barnard +2

We present preliminary results from a detailed analysis of the X-ray point sources in the XMM-Newton survey of M31. These sources are expected to be mostly X-ray binaries. We have…