Fundamental X-ray corona parameters of <i>Swift</i>/<i>BAT</i> AGN

While X-ray emission from active galactic nuclei (AGN) is common, the detailed physics behind this not well understood. This in part because high quality broadband spectra are required to precisely derive fundamental parameters of such as photon index, folding energy, and reflection coefficient. Here we present values for 33 AGN observed 105 month Swift/BAT campaign with coordinated archival XMM-Newton NuSTAR observations. We look correlations between various coronal addition physical properties black hole mass Eddington ratio. Using our empirical model, find good fits almost all objects. The energy was constrained 30 When comparing Seyfert 1 - 1.9 2 galaxies, a K-S test indicates that have lower ratios indices than objects p-values $5.6 \times 10^{-5}$ $7.5 10^{-3}$ respectively. recover known correlation index coefficient Baldwin effect. Finally, inclusion Swift BAT data significantly reduces uncertainties spectral compared without data.