The soft X-ray excess AGN RE J2248-511

@article{Starling2006TheSX,
  title={The soft X-ray excess AGN RE J2248-511},
  author={Rhaana L. C. Starling and Elizabeth Puchnarewicz and Encarni Romero-Colmenero},
  journal={arXiv: Astrophysics},
  year={2006},
  pages={1306-1309}
}
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. 

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