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Gamma-Ray Bursts observed by XMM-Newton
P. T. O'Brien, J. N. Reeves, D. Watson +2
Analysis of observations with XMM-Newton have made a significant contribution to the study of Gamma-ray Burst (GRB) X-ray afterglows. The effective area, bandpass and resolution of…
Tracing a Z-track in the M31 X-ray Binary RX J0042.6+4115
R. Barnard, U. Kolb, J. P. Osborne
Four XMM-Newton observations of the core of M31, spaced at 6 month intervals, show that the brightest point X-ray source, RX J0042.6+4115, has a 0.4-10 keV luminosity of ~5 10^38 e…
The X-ray, optical and radio evolution of the GRB030329 afterglow and the associated SN2003dh
R. Willingale, J. P. Osborne, P. T. O'Brien +3
Extensive X-ray, optical and radio observations of the bright afterglow of the Gamma Ray Burst GRB 030329 are used to construct the multi-frequency evolution of the event. The data…
RX J0042.3+4115: a stellar mass black hole binary identified in M31
R. Barnard, J. P. Osborne, U. Kolb +1
Four XMM-Newton X-ray observations of the central region of the Andromeda Galaxy (M31) have revealed an X-ray source that varies in luminosity over \~1--3, 10^{38} erg s^{-1} betwe…