Optical Spectroscopic Follow-up Of Hard X-ray Sources In The Xmm-slew Survey (original) (raw)

Optical Spectroscopic Follow-up Of Hard X-ray Sources In The Xmm-slew Survey

2007

Abstract

The XMM Slew Survey is projected to cover 80% of the sky in the soft (0.5--2 keV) and hard (2--10 keV) bands. The survey has a flux limit of 4 × 10-12 erg s-1 cm-2 in the hard band. Like all hard-band surveys, it has the ability to detect even heavily absorbed AGN, and the large area coverage makes it

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