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This article is an erratum for:

Volume 565, May 2014
Article Number C1
Number of page(s) 1
Section Extragalactic astronomy
Published online 05 May 2014

The exponent of the units on the y-axis of Fig. 4 is incorrect. A corrected version of the figure is presented here.

thumbnail Fig. 4

Confidence intervals for the energies and normalisations of the three narrow emission lines used to fit the bump between 6.25 and 7.15 keV. The solid, dashed, and dotted contours correspond to 1, 2, and 3σ confidence for two interesting parameters, respectively. The solid vertical lines indicate the expected energy for Fe I, Fe XXV, and Fe XXVI.


We thank Andrew Young for bringing this mistake to our attention.

© ESO, 2014

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