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The XMM-Newton Slew Survey: towards the XMMSL1 catalogue

M. P. Esquej·B. Altieri·D. Bermejo·M. J. Freyberg·V. Lazaro·A. M. Read·R. D. Saxton
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Abstract

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 detectors. It performs slewing manoeuvers between observation targets tracking almost circular orbits through the ecliptic poles due to the Sun constraint. Slews are made with the EPIC cameras open and the other instruments closed, operating with the observing mode set to the one of the previous pointed observation and the medium filter in place. Slew observations from the EPIC-pn camera in FF, eFF and LW modes provide data, resulting in a maximum of 15 seconds of on-source time. These data can be used to give a uniform survey of the X-ray sky, at great sensitivity in the hard band compared with other X-ray all-sky surveys.

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M. P. Esquej, B. Altieri, D. Bermejo, M. J. Freyberg, V. Lazaro, A. M. Read, R. D. Saxton. 2005-11-15. The XMM-Newton Slew Survey: towards the XMMSL1 catalogue. https://arxiv.org/abs/astro-ph/0511435

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