Volume 527, March 2011
|Number of page(s)||2|
|Section||Cosmology (including clusters of galaxies)|
|Published online||26 January 2011|
LoCuSS: comparison of observed X-ray and lensing galaxy cluster scaling relations with simulations (Corrigendum)
Max-Planck-Institut für extraterrestrische Physik,
2 Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
3 University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, USA
4 OAMP, Laboratoire d’Astrophysique de Marseille, traverse du Siphon, 13012 Marseille, France
5 School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B152 TT, UK
6 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
7 Astronomical institute, Tohoku University, Aramaki, Aoba-ku, Sendai, 980-8578, Japan
The article by Zhang et al. (2008, A&A, 482, 451) contains an error in Table A.1 in online material (p. 3). In preparing the final version of Table A.1, we inadvertently used the wrong conversion from degree to hh:mm:ss, with the result that the cluster coordinates were not correctly tabulated in Table A.1. We note that this does not affect any results in Zhang et al. (2008). Nevertheless, we regret this error and provide the actual cluster coordinates used in our analysis in Table A.1 in the following page.
Key words: cosmology: observations / galaxies: clusters: general / X-rays: galaxies: clusters / dark matter / gravitational lensing / errata, addenda
© ESO, 2011
The authors would like to thank Bradford Benson and Marion Schmitz for pointing out this error in the manuscript.
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