Absorbed AGN Detected by the First Swift/BAT Hard X-ray Survey

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Scientific paper

We present results from the the Swift Burst Alert Telescope (BAT) high galactic latitude survey in the 14--200 keV band. The survey reaches a flux of ˜ 10-11 erg cm-2 s-1 and has ˜ 2.7' (90% confidence) positional uncertainties for the faintest sources. This represents the most sensitive survey to date (by a factor of ˜ 10) in this energy band.
Based on the first 3 months of observations, we have identified 86% of the 66 high-latitude sources. 12 are galactic type sources and 44 can be identified with previously known AGN. All but 5 of the AGN have archival X-ray spectra, enabling the estimation of line of sight column densities and other spectral properties. The median redshift (excluding radio-loud objects) is 0.012. We find that the column density distribution of these AGN is bimodal with 64% of the non-blazar sources having column densities NH ≥ 1022 cm-2. None of the sources with log LX>43.5 show high column densities and very few of the lower LX sources have low column densities. We will present results based on improved analysis and larger exposure times.

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