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The XMM-Newton Slew Survey: a wide-angle survey in the 0.2 - 12 keV band
M. J. Freyberg, B. Altieri, D. Bermejo +4
The scientific data collected during slews of the XMM-Newton satellite are used to construct a slew survey catalogue. This comprises of the order of 4000 sources detected in the EP…
XMM-Newton observations of the microquasars GRO J1655-40 and GRS 1915+105
Gloria Sala, Jochen Greiner, Frank Haberl +4
We present results of a sequence of XMM-Newton observations of the two microquasars GRO J1655-40 and GRS 1915+105. The observations were preformed using the EPIC-pn camera in the B…
The XMM-Newton Slew Survey: towards the XMMSL1 catalogue
M. P. Esquej, B. Altieri, D. Bermejo +4
The XMM-Newton satellite is the most sensitive X-ray observatory flown to date due to the great collecting area of its mirrors coupled with the high quantum efficiency of the EPIC…
Status of the XMM-Newton cross-calibration with SASv6.5.0
M. Stuhlinger, B. Altieri, D. Baskill +16
Further achievements of the XMM-Newton cross-calibration - XMM internal as well as with other X-ray missions - are presented. We explain the major changes in the new version SASv6.…
Extended sources in the XMM-Newton slew survey
V. Lazaro, R. Saxton, A. M. Read +4
The low background, good spatial resolution and great sensitivity of the EPIC-pn camera on XMM-Newton give useful limits for the detection of extended sources even during the short…
Processing challenges in the XMM-Newton slew survey
R. Saxton, B. Altieri, A. Read +3
The great collecting area of the mirrors coupled with the high quantum efficiency of the EPIC detectors have made XMM-Newton the most sensitive X-ray observatory flown to date. Thi…