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We present results from an analysis of the broad-band, 0.3-195 keV, X-rayspectra of 48 Seyfert 1-1.5 sources detected in the very hard X-rays with theSwift Burst Alert Telescope (BAT). This sample is selected in an all-sky surveyconducted in the 14-195 keV band. Therefore, our sources are largely unbiasedtowards both obscuration and host galaxy properties. Our detailed and uniformmodel fits to Suzaku/BAT and XMM-Newton/BAT spectra include the neutralabsorption, direct power-law, reflected emission, soft excess, warm absorption,and narrow Fe K-alpha emission properties for the entire sample. Wesignificantly detect O VII and O VIII edges in 52% of our sample. The strengthof these detections are strongly correlated with the neutral column densitymeasured in the spectrum. Among the strongest detections, X-ray grating and UVobservations, where available, indicate outflowing material. The ionized columndensities of sources with O VII and O VIII detections are clustered in a narrowrange with N$_{\rm warm} \sim 10^{21}$\,cm$^{-2}$, while sources without strongdetections have column densities of ionized gas an order of magnitude lower.Therefore, we note that sources without strong detections likely have warmionized outflows present but at low column densities that are not easily probedwith current X-ray observations. Sources with strong complex absorption have astrong soft excess, which may or may not be due to difficulties in modeling thecomplex spectra of these sources. Still, the detection of a flat Gamma ~ 1 anda strong soft excess may allow us to infer the presence of strong absorption inlow signal-to-noise AGN spectra. Additionally, we include a useful correctionfrom the Swift BAT luminosity to bolometric luminosity, based on a comparisonof our spectral fitting results with published spectral energy distributionfits from 33 of our sources.

The Swift BAT-detected Seyfert 1 Galaxies: X-ray Broadband Properties and Warm Absorbers