89 citations · 505 across the 24 of their papers we have counts for
10 papers · 1 filter
The XMM-Newton Serendipitous Survey V. Optical identification of the XMM-Newton Medium sensitivity Survey (XMS)
X. Barcons, F. J. Carrera, M. T. Ceballos +53
We present the XMM-Newton Medium sensitivity Survey (XMS), including a total of 318 X-ray sources found among the serendipitous content of 25 XMM-Newton target fields. The XMS comp…
The behaviour of quiescent accretion discs in dwarf novae
M. R. Truss, G. A. Wynn, P. J. Wheatley
We propose a simple explanation for the constant mean brightness observed between outbursts in dwarf novae. Secular changes in the total energy dissipation rate of the accretion di…
XMM-Newton detection of Nova Muscae 1991 in Quiescence
F. K. Sutaria, U. Kolb, P. A. Charles +7
The soft X-ray transient GU Mus has been detected by XMM-Newton in the quiescent state. The source is very faint, with a 0.5-10.0 keV unabsorbed flux of $\simeq 1.1 \times 10^{-14}…
The XMM-Newton Serendipitous Survey. II. First results from the AXIS high galactic latitude medium sensitivity survey
X. Barcons, F. J. Carrera, M. G. Watson +25
We present the first results on the identifications of a medium sensitivity survey (X-ray flux limit 2E-14 erg/cm2/s in the 0.5-4.5 keV band) at high galactic latitude (|b|>20 deg)…
ASCA X-ray observations of the disk wind in the dwarf nova Z Camelopardalis
D. S. Baskill, P. J. Wheatley, J. P. Osborne
We present ASCA observations of the dwarf nova Z Camelopardalis during outburst and during a transition from quiescence to another outburst. At the beginning of the transition the…
A ROSAT WFC observation of SW UMa: the EUV behaviour of dwarf novae in superoutburst explained
M. R. Burleigh, J. P. Pye, S. W. Poulton +3
During re-processing and analysis of the entire ROSAT Wide Field Camera (WFC) pointed observations database, we discovered a serendipitous, off-axis detection of the cataclysmic va…