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The soft X-ray excess AGN RE J2248-511

R. L. C. Starling·E. M. Puchnarewicz·E. Romero-Colmenero
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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.

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R. L. C. Starling, E. M. Puchnarewicz, E. Romero-Colmenero. 2004-03-01. The soft X-ray excess AGN RE J2248-511. https://doi.org/10.1142/9789812704030_0095

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