Volume 527, March 2011
|Number of page(s)||2|
|Section||Cosmology (including clusters of galaxies)|
|Published online||26 January 2011|
X-ray properties in massive galaxy clusters: XMM-Newton observations of the REFLEX-DXL sample (Corrigendum)
Max-Planck-Institut für extraterrestrische Physik,
2 National Museum of Emerging Science and Innovation, Tokyo, Japan
3 Tokyo University of Science, Tokyo, Japan
4 INAF – Osservatorio Astronomico di Brera, Merate/Milano, Italy
5 Liverpool John Moores University, Liverpool, UK
The article by Zhang et al. (2006, A&A, 456, 55) contains an error in Fig. 5 on page 64, in which we inadvertently re-called the mass distribution of RXCJ0528.9−3972. We note that this does not affect any results in Zhang et al. (2006). Nevertheless, we regret this error and provide an update of Fig. 5 here.
Key words: cosmology: observations / galaxies: clusters: general / X-rays: galaxies: clusters / dark matter / errata, addenda
© ESO, 2011
Measured mass profiles of the REFLEX-DXL clusters and their best fits by the extended-NFW models. Residuals scaled by the data uncertainties are plotted in the upper part of the diagrams.
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