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ERRATUM: "SURVEYING THE AGENTS OF GALAXY EVOLUTION IN THE TIDALLY STRIPPED, LOW-METALLICITY SMALL MAGELLANIC CLOUD (SAGE-SMC). II. COOL EVOLVED STARS" (2011, AJ, 142, 103)

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Published 2012 April 16 © 2012. The American Astronomical Society. All rights reserved.
, , Citation Martha L. Boyer et al 2012 AJ 143 127 DOI 10.1088/0004-6256/143/5/127

This is a correction for 2011 AJ 142 103

1538-3881/143/5/127

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In Table 4 of the original paper, the H- and Ks-band magnitudes of evolved stars in the Small Magellanic Cloud are reversed. The printed version of Table 4 (a sample of the full table) is not affected since it does not include near-infrared magnitudes. The full corrected table is available in the electronic version of this erratum.

Table 4. Sample of Evolved Stars and FIR Objects in SMC

 

Only a portion of this table is shown here to demonstrate its form and content. Machine-readable and Virtual Observatory (VO) versions of the full table are available.

Download table as:  Machine-readable (MRT)Virtual Observatory (VOT)Typeset image

We thank Ciska Kemper, Mei-Chun Lin, and Paul Ruffle for bringing this mix-up to our attention.

10.1088/0004-6256/143/5/127