Abstract
The spectrum of the hard X-ray background records the history of accretion processes integrated over the cosmic time. Several pieces of observational and theoretical evidence indicate that a significant fraction of the energy density is obscured by large columns of gas and dust. The absorbing matter is often very thick, with column densities exceeding N H ≃ 1.5 × 1024 cm-2, the value corresponding to unity optical depth for Compton scattering. These sources are called “Compton thick” and appear to be very numerous, at least in the nearby universe. Although Compton-thick Active Galactic Nuclei (AGN) are thought to provide an important contribution to the overall cosmic energy budget, their space density and cosmological evolution are poorly known. The properties of Compton-thick AGN are reviewed here, with particular emphasis on their contributions to the extragalactic background light in the hard X-ray and infrared bands.
Partially supported by the Italian Space Agency (ASI) under grants IR/073/O1 and I/R/057/02, by the MIUR grant Cofin-03-02-23, and by the INAF grant 270/2003
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Comastri, A. (2004). Compton-Thick AGN: The Dark Side of the X-Ray Background. In: Barger, A.J. (eds) Supermassive Black Holes in the Distant Universe. Astrophysics and Space Science Library, vol 308. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2471-9_8
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