The soft X-ray excess AGN RE J2248-511
arXiv:astro-ph/0403008 · doi:10.1142/9789812704030_0095
Abstract
We model the spectral energy distribution of the ultrasoft broad-line AGN RE J2248-511 with Comptonised accretion disc models. These are able to reproduce the steep optical and ultrasoft X-ray slopes, and the derived black hole mass is consistent with independent mass estimates. This AGN displays properties of both broad and narrow line Seyfert 1 galaxies, but we conclude that it is intrinsically a `normal' Seyfert 1 viewed at high inclination angle.
4 pages, 1 figure. MG10 Proceedings