X-ray Colours of AGN in the 13h XMM/Chandra Deep Field

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We present results of a Monte Carlo analysis of the X-ray colours of
sources in our very deep XMM-Newton imaging. Using detailed simulations,
we test published models of the distribution of absorbing column
densities against the observed data. The 2D-KS test finds that model B
of [2] and the β = 8 model of [1] are preferred.

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