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ERRATUM: "ON THE 10 μm SILICATE FEATURE IN ACTIVE GALACTIC NUCLEI" (2009, ApJ, 707, 1550)

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Published 2010 October 26 © 2010. The American Astronomical Society. All rights reserved.
, , Citation Robert Nikutta et al 2010 ApJ 723 1828 DOI 10.1088/0004-637X/723/2/1828

This is a correction for 2009 ApJ 707 1550

0004-637X/723/2/1828

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Erratum. 

The torus models used in the published version of this article carried an erroneous scale due to a bug discovered in the calculation code that was used in Nenkova et al. (2008b; see also the erratum to that article). The spectral shapes of the models were not affected, only the absolute flux levels. The impact on this paper is minor. The luminosity of source SST1721+6012 in Section 2.5 of the published article, which was derived from the best-fit model, was reported as L12 = LAGN/1012L = 3.47. The corrected value is now L12 = 0.90. Additionally, in the last paragraph of that section the earlier estimate of Lacy et al. (2007b), together with the bolometric correction from Richards et al. (2006), was mistyped as L12 ∼ 4, but should have been L12 ∼ 2. This is in even closer agreement with our corrected value of L12 = 0.90.

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10.1088/0004-637X/723/2/1828