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arXiv · 0912.3146

The XMM-Newton Slew Survey: Towards The Whole X-ray Sky and the Rarest X-ray Events

A. M. Read·R. D. Saxton·P. Esquej·R. S. Warwick
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Abstract

The data collected by XMM-Newton as it slews between pointings currently cover almost half the entire sky, and many familiar features and new sources are visible. The soft-band sensitivity limit of the Slew is close to that of the RASS, and a large-area Slew-RASS comparison now provides the best opportunity for discovering extremely rare high-variability objects.

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A. M. Read, R. D. Saxton, P. Esquej, R. S. Warwick. 2009-12-16. The XMM-Newton Slew Survey: Towards The Whole X-ray Sky and the Rarest X-ray Events. https://doi.org/10.1063/1.3475320

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